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	<id>https://wiki.uni-due.de/agk/api.php?action=feedcontributions&amp;feedformat=atom&amp;user=Vardan</id>
	<title>Arbeitsgruppe Kuiper - User contributions [en]</title>
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	<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Special:Contributions/Vardan"/>
	<updated>2026-05-02T07:46:20Z</updated>
	<subtitle>User contributions</subtitle>
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	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Paper_policies&amp;diff=709</id>
		<title>Paper policies</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Paper_policies&amp;diff=709"/>
		<updated>2025-02-04T15:29:02Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Literature on &amp;quot;Writing Research Papers&amp;quot; and &amp;quot;English for Academic Research&amp;quot; ==&lt;br /&gt;
There are probably tons of books and resources on this topic, but I&#039;ve read some books of this author and find them quite useful: [https://adrianwallwork.wordpress.com/english-for-research/ Adrian Wallwork]&lt;br /&gt;
&lt;br /&gt;
== A&amp;amp;A ==&lt;br /&gt;
* &#039;&#039;&#039;Language editing guide&#039;&#039;&#039; for A&amp;amp;A can be found [https://www.aanda.org/for-authors/language-editing/1-introduction here]&lt;br /&gt;
* A&amp;amp;A uses the &#039;&#039;&#039;past tense&#039;&#039;&#039; to describe the specific steps used in a paper and the &#039;&#039;&#039;present tense&#039;&#039;&#039; to describe general methods and recent findings.&lt;br /&gt;
&lt;br /&gt;
* All &#039;&#039;&#039;abbreviations and acronyms&#039;&#039;&#039; are introduced at first use, &#039;&#039;&#039;once in the Abstract and again in the main text&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Quote marks&#039;&#039;&#039; should not be used for emphasis. If you are indicating that a word is being used in an unusual way or with a special meaning, the quote marks can remain (‘single’ quote marks in UK convention, “double” in US), but only for the first use. All subsequent uses of the word should be without quote marks.&lt;br /&gt;
&lt;br /&gt;
* When &#039;&#039;&#039;listing two references&#039;&#039;&#039; in the running text of a sentence (i.e. not in brackets), use &amp;quot;and&amp;quot; between two references, not &amp;quot;;&amp;quot;. With &#039;&#039;&#039;three or more&#039;&#039;&#039; the references must be separated by commas and the last reference set off with &amp;quot;and&amp;quot;: ref1, ref2, and ref3.&lt;br /&gt;
&lt;br /&gt;
* Start with a &#039;&#039;&#039;brief title for the figure&#039;&#039;&#039; as a whole before describing the individual panels.&lt;br /&gt;
&lt;br /&gt;
* Slashes ( / ) are used in equations, and to denote ratios, instrument pairings, and wavelength ranges (e.g., optical/UV). All other appearances should be removed and the sentence rephrased. You can substitute &amp;quot;and&amp;quot;, &amp;quot;or&amp;quot;, &amp;quot;and/or&amp;quot;, or a double hyphen (which can be used to indicate a range or dual nature: Hertzsprung–Russell diagram).&lt;br /&gt;
&lt;br /&gt;
* Only use the ~ sign with a number and unit combo: ~5 km.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Table Captions:&#039;&#039;&#039; Titles should be short and placed above the table. Descriptions and references should be moved to a &amp;quot;Notes:&amp;quot; section below the table. See [https://www.aanda.org/for-authors/latex-issues/latex-examples A&amp;amp;A Table Guideline]s for details.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Titles &amp;amp; Headings:&#039;&#039;&#039; Use lowercase for all titles (main title, sections, subsections, appendices, tables), except for the first word and proper nouns.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Figures:&#039;&#039;&#039; Remove all background grids in accordance with A&amp;amp;A&#039;s graphic policy.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Abbreviations &amp;amp; Acronyms:&#039;&#039;&#039;&lt;br /&gt;
** Do not start a sentence with an abbreviation. If necessary, add an article (e.g., &amp;quot;The NASA mission&amp;quot;) or spell it out.&lt;br /&gt;
** Use e.g. and i.e. only in parentheses or figure/table legends. In the main text, use alternatives like &amp;quot;for example&amp;quot; (instead of e.g.) or &amp;quot;that is&amp;quot; (instead of i.e.). UK style does not use a comma after e.g. and i.e. (e.g. i.e.), while US style does (e.g., i.e.,).&lt;br /&gt;
** Always abbreviate Sect., Fig., Eq., and Col. when referring to a specific item, except at the beginning of a sentence where they should be written in full.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Spell Check:&#039;&#039;&#039; Run a spell check based on your preferred language (US or UK English).&lt;br /&gt;
&lt;br /&gt;
== nature ==&lt;br /&gt;
&lt;br /&gt;
TO DO&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Paper_policies&amp;diff=708</id>
		<title>Paper policies</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Paper_policies&amp;diff=708"/>
		<updated>2025-02-04T15:15:12Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* A&amp;amp;A */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== A&amp;amp;A ==&lt;br /&gt;
* &#039;&#039;&#039;Language editing guide&#039;&#039;&#039; for A&amp;amp;A can be found here [https://www.aanda.org/for-authors/language-editing/1-introduction]&lt;br /&gt;
* A&amp;amp;A uses the &#039;&#039;&#039;past tense&#039;&#039;&#039; to describe the specific steps used in a paper and the &#039;&#039;&#039;present tense&#039;&#039;&#039; to describe general methods and recent findings.&lt;br /&gt;
&lt;br /&gt;
* All &#039;&#039;&#039;abbreviations and acronyms&#039;&#039;&#039; are introduced at first use, &#039;&#039;&#039;once in the Abstract and again in the main text&#039;&#039;&#039;.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Quote marks&#039;&#039;&#039; should not be used for emphasis. If you are indicating that a word is being used in an unusual way or with a special meaning, the quote marks can remain (‘single’ quote marks in UK convention, “double” in US), but only for the first use. All subsequent uses of the word should be without quote marks.&lt;br /&gt;
&lt;br /&gt;
* When &#039;&#039;&#039;listing two references&#039;&#039;&#039; in the running text of a sentence (i.e. not in brackets), use &amp;quot;and&amp;quot; between two references, not &amp;quot;;&amp;quot;. With &#039;&#039;&#039;three or more&#039;&#039;&#039; the references must be separated by commas and the last reference set off with &amp;quot;and&amp;quot;: ref1, ref2, and ref3.&lt;br /&gt;
&lt;br /&gt;
* Start with a &#039;&#039;&#039;brief title for the figure&#039;&#039;&#039; as a whole before describing the individual panels.&lt;br /&gt;
&lt;br /&gt;
* Slashes ( / ) are used in equations, and to denote ratios, instrument pairings, and wavelength ranges (e.g., optical/UV). All other appearances should be removed and the sentence rephrased. You can substitute &amp;quot;and&amp;quot;, &amp;quot;or&amp;quot;, &amp;quot;and/or&amp;quot;, or a double hyphen (which can be used to indicate a range or dual nature: Hertzsprung–Russell diagram).&lt;br /&gt;
&lt;br /&gt;
* Only use the ~ sign with a number and unit combo: ~5 km.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Table Captions:&#039;&#039;&#039; Titles should be short and placed above the table. Descriptions and references should be moved to a &amp;quot;Notes:&amp;quot; section below the table. See [https://www.aanda.org/for-authors/latex-issues/latex-examples A&amp;amp;A Table Guideline]s for details.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Titles &amp;amp; Headings:&#039;&#039;&#039; Use lowercase for all titles (main title, sections, subsections, appendices, tables), except for the first word and proper nouns.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Figures:&#039;&#039;&#039; Remove all background grids in accordance with A&amp;amp;A&#039;s graphic policy.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Abbreviations &amp;amp; Acronyms:&#039;&#039;&#039;&lt;br /&gt;
** Do not start a sentence with an abbreviation. If necessary, add an article (e.g., &amp;quot;The NASA mission&amp;quot;) or spell it out.&lt;br /&gt;
** Use e.g. and i.e. only in parentheses or figure/table legends. In the main text, use alternatives like &amp;quot;for example&amp;quot; (instead of e.g.) or &amp;quot;that is&amp;quot; (instead of i.e.). UK style does not use a comma after e.g. and i.e. (e.g. i.e.), while US style does (e.g., i.e.,).&lt;br /&gt;
** Always abbreviate Sect., Fig., Eq., and Col. when referring to a specific item, except at the beginning of a sentence where they should be written in full.&lt;br /&gt;
&lt;br /&gt;
* &#039;&#039;&#039;Spell Check:&#039;&#039;&#039; Run a spell check based on your preferred language (US or UK English).&lt;br /&gt;
&lt;br /&gt;
== nature ==&lt;br /&gt;
&lt;br /&gt;
TO DO&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=657</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=657"/>
		<updated>2024-08-23T08:01:31Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Planets */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al. 2023, [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Usmanov et al. 2012, [https://iopscience.iop.org/article/10.1088/0004-637X/754/1/40 &amp;quot;Three-Dimensional Magnetohydrodynamic Modeling of the Solar Wind Including Pickup Protons and Turbulence Transport&amp;quot;] (superimposed grids to avoid the coordinate singularity at the poles)&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* Cecil, Gehrig &amp;amp; Steiner 2024, [https://arxiv.org/abs/2405.05816 &amp;quot;Time-dependent long-term hydrodynamic simulations of the inner protoplanetary disk III: The influence of photoevaporation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fenton &amp;amp; Stamatellos 2024, [https://arxiv.org/abs/2402.01432 &amp;quot;The 3D structure of disc-instability protoplanets&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Takakuwa et al. 2024, [https://arxiv.org/abs/2401.08722 &amp;quot;Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024, [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
&lt;br /&gt;
* Lega et al. 2024, [https://arxiv.org/abs/2408.12233 &amp;quot;Gas dynamics around a Jupiter-mass planet I. Influence of protoplanetary disk properties&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Zhang 2024, [https://iopscience.iop.org/article/10.3847/2515-5172/ad4481 &amp;quot;Initial Entropy and Potential Delayed Formation of the Directly Imaged Exoplanet AF Lep b&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Savignac &amp;amp; Lee 2024, [https://arxiv.org/abs/2310.06013 &amp;quot;The Not-So Dramatic Effect of Advective Flows on Gas Accretion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Krapp et al. 2024, [https://arxiv.org/abs/2402.14638 &amp;quot;A thermodynamic criterion for the formation of Circumplanetary Disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Andama et al. 2024, [https://arxiv.org/abs/2401.16155 &amp;quot;What stars can form planets: planetesimal formation at low&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 &amp;quot;Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lorek &amp;amp; Johansen 2024, [https://arxiv.org/abs/2401.05101 &amp;quot;Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 &amp;quot;A radius valley between migrated steam worlds and evaporated rocky cores&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/abs/2401.09657 &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/abs/2401.06217 &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;br /&gt;
* Keto (2020), [https://doi.org/10.1093/mnras/staa529 &amp;quot;Stability and solution of the time-dependent Bondi–Parker flow&amp;quot;]&lt;br /&gt;
* Bratley &amp;amp; Fox (1988), [https://doi.org/10.1145/42288.214372 &amp;quot;Algorithm 659: Implementing Sobol&#039;s quasirandom sequence generator&amp;quot;]&lt;br /&gt;
* Smith (1987), [https://doi.org/10.1090/QAM%2F910459 &amp;quot;A note on the Stokes paradox&amp;quot;]&lt;br /&gt;
* Davis (1959), [https://doi.org/10.1080/00029890.1959.11989422 &amp;quot;Leonhard Euler&#039;s Integral: A Historical Profile of the Gamma Function&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Talk:Restarting_belt_automatically&amp;diff=623</id>
		<title>Talk:Restarting belt automatically</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Talk:Restarting_belt_automatically&amp;diff=623"/>
		<updated>2024-07-03T22:25:05Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Hi Vardan, that applies to magnitude and amplitude, right? --[[User:Lothar.brendel|Lothar]] ([[User talk:Lothar.brendel|talk]]) 12:09, 3 July 2024 (CEST)&lt;br /&gt;
: Hi Lothar. I tested it only on magnitUDE so far, but should work on the both clusters. --[[User:Vardan|Vardan]] ([[User talk:Vardan|talk]]) 14:21, 3 July 2024&lt;br /&gt;
:: I thought so, because you need such a &#039;&#039;chain job&#039;&#039; only on systems with time limited queues/partitions. Regarding your approach, having to specify the script name explicitly (&amp;lt;code&amp;gt;sbatch submit&amp;lt;/code&amp;gt;) seems somewhat error-prone to me (forgetting to change the line after renaming the script). An (admittedly clumsy looking ;-) alternative would be&amp;lt;br&amp;gt;&amp;lt;code&amp;gt;scontrol show job $SLURM_JOB_ID | awk -F= &#039;/^ *Command/{print $2}&#039; | xargs sbatch&amp;lt;/code&amp;gt;&amp;lt;br&amp;gt;If one never changes the job name, a simple &amp;lt;code&amp;gt;sbatch $SLURM_JOB_NAME&amp;lt;/code&amp;gt; would do the trick. --[[User:Lothar.brendel|Lothar]] ([[User talk:Lothar.brendel|talk]]) 15:34, 3 July 2024 (CEST)&lt;br /&gt;
::: Yes, sure. I&#039;m usually not changing the name of the submit file, but of course your option is much better.&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Talk:Restarting_belt_automatically&amp;diff=612</id>
		<title>Talk:Restarting belt automatically</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Talk:Restarting_belt_automatically&amp;diff=612"/>
		<updated>2024-07-03T12:21:33Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Hi Vardan, that applies to magnitude and amplitude, right? --[[User:Lothar.brendel|Lothar]] ([[User talk:Lothar.brendel|talk]]) 12:09, 3 July 2024 (CEST)&lt;br /&gt;
&lt;br /&gt;
Hi Lothar. I tested it only on magnitUDE so far, but should work on the both clusters. --Vardan&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Talk:Restarting_belt_automatically&amp;diff=611</id>
		<title>Talk:Restarting belt automatically</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Talk:Restarting_belt_automatically&amp;diff=611"/>
		<updated>2024-07-03T12:21:21Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Hi Vardan, that applies to magnitude and amplitude, right? --[[User:Lothar.brendel|Lothar]] ([[User talk:Lothar.brendel|talk]]) 12:09, 3 July 2024 (CEST)&lt;br /&gt;
&lt;br /&gt;
Hi Lothar. I tested it only on magnitUDE so far, but should work on the both clusters.&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Restarting_belt_automatically&amp;diff=609</id>
		<title>Restarting belt automatically</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Restarting_belt_automatically&amp;diff=609"/>
		<updated>2024-07-03T09:51:32Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Add the following script to your submit script to automatically restart belt from the last output file.&lt;br /&gt;
&lt;br /&gt;
&amp;lt;code&amp;gt;&lt;br /&gt;
latest=$(ls -l data | grep -o &amp;quot;rho\.[0-9]*\.dbl&amp;quot; | grep -oE &amp;quot;[0-9]*&amp;quot; | sort -g -r | head -n 1)&lt;br /&gt;
&lt;br /&gt;
timeout 95h mpirun -np 864 ./belt -restart $latest&lt;br /&gt;
&lt;br /&gt;
if [[ $? == 124 ]]; then&lt;br /&gt;
 sbatch submit&lt;br /&gt;
fi&lt;br /&gt;
&amp;lt;/code&amp;gt;&lt;br /&gt;
&lt;br /&gt;
In the above example, the code will be terminated after 95 hours and the submit file called &amp;quot;submit&amp;quot; will be resubmitted. Note that you need to have SBATCH time of at least 95 hours for this script to work. Otherwise, the SBATCH system will terminate your code with the different exit code (probably), and it will not be restarted. So, #SBATCH -t 4-00:00:00 option should be used.&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Restarting_belt_automatically&amp;diff=608</id>
		<title>Restarting belt automatically</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Restarting_belt_automatically&amp;diff=608"/>
		<updated>2024-07-03T09:47:20Z</updated>

		<summary type="html">&lt;p&gt;Vardan: Created page with &amp;quot;Add the following script to your submit script to automatically restart belt from the last output file.  latest=$(ls -l data | grep -o &amp;quot;rho\.[0-9]*\.dbl&amp;quot; | grep -oE &amp;quot;[0-9]*&amp;quot; | sort -g -r | head -n 1)  timeout 95h mpirun -np 864 ./belt -restart $latest   if  $? == 124 ; then    sbatch submit fi  In the above example, the code will be terminated after 95 hours and the submit file called &amp;quot;submit&amp;quot; will be resubmitted. Note that you need to have SBATCH time of at least 95...&amp;quot;&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Add the following script to your submit script to automatically restart belt from the last output file.&lt;br /&gt;
&lt;br /&gt;
latest=$(ls -l data | grep -o &amp;quot;rho\.[0-9]*\.dbl&amp;quot; | grep -oE &amp;quot;[0-9]*&amp;quot; | sort -g -r | head -n 1)&lt;br /&gt;
&lt;br /&gt;
timeout 95h mpirun -np 864 ./belt -restart $latest  &lt;br /&gt;
if [[ $? == 124 ]]; then &lt;br /&gt;
  sbatch submit&lt;br /&gt;
fi&lt;br /&gt;
&lt;br /&gt;
In the above example, the code will be terminated after 95 hours and the submit file called &amp;quot;submit&amp;quot; will be resubmitted. Note that you need to have SBATCH time of at least 95 hours for this script to work. Otherwise, the SBATCH system will terminate your code with the different exit code (probably), and it will not be restarted. So, #SBATCH -t 4-00:00:00 option should be used.&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Software&amp;diff=607</id>
		<title>Software</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Software&amp;diff=607"/>
		<updated>2024-07-03T09:38:45Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Overview */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;== Overview ==&lt;br /&gt;
* Astro stuff:&lt;br /&gt;
** [https://git.uni-due.de/agkuiper/belt Belt] (which needs [[PETSc]]): Rolf&#039;s PLUTO version ([[compile-belt|manual]] for compiling)&lt;br /&gt;
** [[Visit]] Tips and tricks&lt;br /&gt;
** [[pyPLUTO]]: a Python module to read and analyse PLUTO output&lt;br /&gt;
** [[Scaling tests]] (for belt)&lt;br /&gt;
** [[Restarting belt automatically]]&lt;br /&gt;
* Online Tools:&lt;br /&gt;
** a nice, free [https://www.geogebra.org/3d 3D-plotter] (in cases when Mathematica is somehow unavailable)&lt;br /&gt;
* [[Software#Two-Factor Authentification|Two-Factor Authentification (2FA)]]&lt;br /&gt;
* [[VPN]]&lt;br /&gt;
* [[SSH and SCP]]&lt;br /&gt;
* University [[Git#GitLab|GitLab]] (https://git.uni-due.de)&lt;br /&gt;
* [https://uni-due.zoom.us/profile University Zoom]&lt;br /&gt;
* [https://nxcl.e-services.physik.uni-due.de University Nextcloud]: This is where we have the group calendar as well!&lt;br /&gt;
* [https://www.uni-due.de/zim/services/software/office-ma.php MS Office]. Note that [https://www.libreoffice.org/ LibreOffice] (Windows, Linux; use package manager) is an excellent and free alternative but &#039;&#039;caveat emptor&#039;&#039; about some formatting compatibilities.&lt;br /&gt;
* [[Zotero]]&lt;br /&gt;
* Making bibliographies compact (e.g. for proposals): https://github.com/lmytime/tex_compact_bib&lt;br /&gt;
&lt;br /&gt;
== Two-Factor Authentification ==&lt;br /&gt;
The two-factor authentification (2FA) is needed for most university services as VPN or Nextcloud. &lt;br /&gt;
&lt;br /&gt;
After activating your user-ID you need to activate it in the selfcare portal (https://selfcare.uni-due.de/). The website will walk you through the installation. You&#039;ll need to have e.g. an app for the generation of the second factor. I recommend using the app OpenOTP. Please make sure that you scan the shown QR-codes, they are very hard to regain.&lt;br /&gt;
&lt;br /&gt;
However, it is also possible to do it without a phone or application. For this, you only need to install forcepoint and oathtool. Then, you call:&lt;br /&gt;
 ~$ sudo forcepoint-client vpn.uni-due.de&lt;br /&gt;
Enter your normal/central university username and password. Then, if warnings come, say yes, and it will ask you for the second factor. Copy the timestamp for the line &amp;lt;code&amp;gt;*** Please enter reply for challenge ***&amp;lt;/code&amp;gt; and run—in the same terminal after having paused forcepoint (Ctrl+Z, then &amp;quot;bg&amp;quot;, then &amp;lt;Enter&amp;gt;) or in a separate terminal—the following command:&lt;br /&gt;
 ~$ oathtool --totp -b &amp;lt;YOUR &amp;quot;SECRET&amp;quot;&amp;gt; --now=&amp;quot;&amp;lt;TIMESTAMP GIVEN BY FORCEPOINT&amp;gt;&amp;quot;&lt;br /&gt;
It will return a six-digit number that you then give to forcepoint (&amp;lt;code&amp;gt;fg&amp;lt;/code&amp;gt; to bring it back to the foreground, or switching to the tab). You have all the time in the world because you are giving the timestamp explicitly :). You get the &amp;quot;secret&amp;quot; from the selfcare portal when you generate a token (the QR code is just an URL and there is a &amp;quot;…?secret=…&amp;amp;&amp;quot; part to it; the string between &amp;quot;=&amp;quot; and &amp;quot;&amp;amp;&amp;quot; is the &amp;quot;secret&amp;quot;).&lt;br /&gt;
&lt;br /&gt;
In general, to parse a QR code: you can use &amp;lt;code&amp;gt;zbarimg&amp;lt;/code&amp;gt;, e.g. from a quick screenshot:&lt;br /&gt;
 ~$ zbarimg &amp;quot;/home/georgeslemaistre/Bilder/Bildschirmfoto von 2023-10-05 15-00-00.png&amp;quot;&lt;br /&gt;
 otpauth://totp/TOTP1938HK33?secret=33IHS343AMDGPH123456CO777JPIIJMJV&amp;amp;period=30&amp;amp;digits=6&amp;amp;issuer=uni-duisburg-essen&amp;amp;image=https%3A//selfcare.uni-due.de/_Resources/Static/Packages/UDE.Portal/images/logo/logo--otp.png&lt;br /&gt;
(No worries, this is a fake &amp;quot;secret&amp;quot; :).)&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;&#039;Important&#039;&#039;&#039;: make sure to execute the oathtool command prefixed with a space on the command line so that it not get saved to your command history file because your &amp;quot;secret&amp;quot; is in plain text there. You can call the command once without writing the &amp;quot;secret&amp;quot; (which of course will not work) just to have the command in the history (searching in the history on the command line: &amp;lt;code&amp;gt;Ctrl&amp;lt;/code&amp;gt;+&amp;lt;code&amp;gt;R&amp;lt;/code&amp;gt;). Typically, you need to close the terminal (exit) for the history actually to be written to the history file (~/.bash_history if you are using bash.) Saving the secret itself in plain text is not the best idea, obviously, so you need to find a solution for that part…&lt;br /&gt;
&lt;br /&gt;
If you forgot to use a space at the beginning of the line and the terminal is still open, go up in command history with the up arrow until you get to that command, delete the command on the line and &#039;&#039;&#039;do not press enter&#039;&#039;&#039; but first go back &amp;quot;down to the present&amp;quot; with the down arrow and &#039;&#039;&#039;then&#039;&#039;&#039; press enter. You can check that it has worked by going back up (with the up arrow) and you will see a blank line where the command was. Then you can exit. If you have already closed the terminal, open the history file in an editor and delete the line but make sure that no back-up copy of the history file (containing the command...) is made, or delete it manually afterwards.&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=138</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=138"/>
		<updated>2024-02-23T09:48:59Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Planets */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* Fenton &amp;amp; Stamatellos 2024, [https://arxiv.org/pdf/2402.01432.pdf &amp;quot;The 3D structure of disc-instability protoplanets&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Takakuwa et al. 2024, [https://arxiv.org/abs/2401.08722 &amp;quot;Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024, [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Krapp et al. 2024, [https://arxiv.org/abs/2402.14638 &amp;quot;A thermodynamic criterion for the formation of Circumplanetary Disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Andama et al. 2024, [https://arxiv.org/abs/2401.16155 &amp;quot;What stars can form planets: planetesimal formation at low&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 &amp;quot;Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lorek &amp;amp; Johansen 2024, [https://arxiv.org/abs/2401.05101 &amp;quot;Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 &amp;quot;A radius valley between migrated steam worlds and evaporated rocky cores&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/pdf/2401.09657.pdf &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=User_talk:Vardan&amp;diff=116</id>
		<title>User talk:Vardan</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=User_talk:Vardan&amp;diff=116"/>
		<updated>2024-02-08T14:59:58Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Hi Vardan, just to test whether you get emails through this. -- Lothar&lt;br /&gt;
&lt;br /&gt;
Hi Lothar, yes, just got an email that you created this page. -- Vardan&lt;br /&gt;
&lt;br /&gt;
Hi Vardan, it seems that email notification doesn&#039;t work properly. Did you get a mail from this? -- Lothar&lt;br /&gt;
&lt;br /&gt;
Hi Lothar, yes, just got an email about the changes on this webpage. --Vardan&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=96</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=96"/>
		<updated>2024-02-05T15:36:42Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* Fenton &amp;amp; Stamatellos 2024, [https://arxiv.org/pdf/2402.01432.pdf &amp;quot;The 3D structure of disc-instability protoplanets&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Takakuwa et al. 2024, [https://arxiv.org/abs/2401.08722 &amp;quot;Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024, [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Andama et al. 2024, [https://arxiv.org/abs/2401.16155 &amp;quot;What stars can form planets: planetesimal formation at low&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 &amp;quot;Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lorek &amp;amp; Johansen 2024, [https://arxiv.org/abs/2401.05101 &amp;quot;Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 &amp;quot;A radius valley between migrated steam worlds and evaporated rocky cores&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/pdf/2401.09657.pdf &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=95</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=95"/>
		<updated>2024-02-05T15:36:22Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* Fenton &amp;amp; Stamatellos 2024, [https://arxiv.org/pdf/2402.01432.pdf &amp;quot;https://arxiv.org/abs/2402.01432&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Takakuwa et al. 2024, [https://arxiv.org/abs/2401.08722 &amp;quot;Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024, [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Andama et al. 2024, [https://arxiv.org/abs/2401.16155 &amp;quot;What stars can form planets: planetesimal formation at low&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 &amp;quot;Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lorek &amp;amp; Johansen 2024, [https://arxiv.org/abs/2401.05101 &amp;quot;Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 &amp;quot;A radius valley between migrated steam worlds and evaporated rocky cores&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/pdf/2401.09657.pdf &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=94</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=94"/>
		<updated>2024-01-30T09:24:23Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Planets */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* Takakuwa et al. 2024, [https://arxiv.org/abs/2401.08722 &amp;quot;Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024, [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Andama et al. 2024, [https://arxiv.org/abs/2401.16155 &amp;quot;What stars can form planets: planetesimal formation at low&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 &amp;quot;Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lorek &amp;amp; Johansen 2024, [https://arxiv.org/abs/2401.05101 &amp;quot;Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 &amp;quot;A radius valley between migrated steam worlds and evaporated rocky cores&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/pdf/2401.09657.pdf &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=91</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=91"/>
		<updated>2024-01-24T09:52:38Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* Takakuwa et al. 2024, [https://arxiv.org/abs/2401.08722 &amp;quot;Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024, [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 &amp;quot;Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lorek &amp;amp; Johansen 2024, [https://arxiv.org/abs/2401.05101 &amp;quot;Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 &amp;quot;A radius valley between migrated steam worlds and evaporated rocky cores&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/pdf/2401.09657.pdf &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=90</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=90"/>
		<updated>2024-01-23T10:56:07Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Planets */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024 [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 &amp;quot;Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lorek &amp;amp; Johansen 2024, [https://arxiv.org/abs/2401.05101 &amp;quot;Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 &amp;quot;A radius valley between migrated steam worlds and evaporated rocky cores&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/pdf/2401.09657.pdf &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=87</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=87"/>
		<updated>2024-01-19T10:41:58Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Planets */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024 [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Jones et al. 2024, [https://arxiv.org/pdf/2401.09657.pdf &amp;quot;A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=86</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=86"/>
		<updated>2024-01-16T08:43:35Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Planets */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024 [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Xu &amp;amp; Wang 2024, [https://arxiv.org/pdf/2401.06217.pdf &amp;quot;Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=85</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=85"/>
		<updated>2024-01-12T19:27:15Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* &lt;br /&gt;
&lt;br /&gt;
* Ren et al. 2024 [https://arxiv.org/abs/2310.15430 &amp;quot;A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 &amp;quot;Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=84</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=84"/>
		<updated>2024-01-12T19:23:31Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Small things */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
*&lt;br /&gt;
* Lim et al 2023, &amp;quot;[https://arxiv.org/abs/2312.12508 Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 &amp;quot;Dust growth and evolution in protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=83</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=83"/>
		<updated>2024-01-12T19:22:25Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
*&lt;br /&gt;
* Lim et al 2023, &amp;quot;[https://arxiv.org/abs/2312.12508 Streaming Instability and Turbulence: Conditions for Planetesimal Formation&amp;quot;]&lt;br /&gt;
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J &amp;quot;Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other (including ornithology) ==&lt;br /&gt;
&lt;br /&gt;
* Van Wassenbergh &amp;amp; Mielke (2024), [https://doi.org/10.1063/PT.3.5385 &amp;quot;Why woodpeckers don’t get concussions&amp;quot;], Physics Today (&#039;&#039;short read&#039;&#039;)&lt;br /&gt;
&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=61</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=61"/>
		<updated>2023-12-19T10:10:29Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other)&lt;br /&gt;
* Within a subject, maybe sort by descending chronological order, to have the newest on top; no need to put a date since the month+year is in the arXiv link (shown when hovering over it)&lt;br /&gt;
* Put comments and discussions on the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Young 2023, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
&lt;br /&gt;
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 &amp;quot;An outburst and FU Ori-type disk of a former low luminosity protostar&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other ==&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=57</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=57"/>
		<updated>2023-12-14T17:09:02Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other)&lt;br /&gt;
* Within a subject, maybe sort by descending chronological order, to have the newest on top; no need to put a date since the month+year is in the arXiv link (shown when hovering over it)&lt;br /&gt;
* Comments+discussions go onto the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Young, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 &amp;quot;VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other ==&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=56</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=56"/>
		<updated>2023-12-14T17:08:37Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other)&lt;br /&gt;
* Within a subject, maybe sort by descending chronological order, to have the newest on top; no need to put a date since the month+year is in the arXiv link (shown when hovering over it)&lt;br /&gt;
* Comments+discussions go onto the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Young, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
* Balmer et al. 2023, [https://arxiv.org/abs/2312.08283 VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”]&lt;br /&gt;
&lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other ==&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=55</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=55"/>
		<updated>2023-12-13T15:18:24Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other)&lt;br /&gt;
* Within a subject, maybe sort by descending chronological order, to have the newest on top; no need to put a date since the month+year is in the arXiv link (shown when hovering over it)&lt;br /&gt;
* Comments+discussions go onto the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Young, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other ==&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=54</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=54"/>
		<updated>2023-12-13T15:18:07Z</updated>

		<summary type="html">&lt;p&gt;Vardan: /* Discs */&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other)&lt;br /&gt;
* Within a subject, maybe sort by descending chronological order, to have the newest on top; no need to put a date since the month+year is in the arXiv link (shown when hovering over it)&lt;br /&gt;
* Comments+discussions go onto the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Young, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other ==&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=53</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=53"/>
		<updated>2023-12-13T15:17:41Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. Please:&lt;br /&gt;
* Indicate the title and some author information&lt;br /&gt;
* Put a link to the &#039;&#039;&#039;abstract page, not to the PDF&#039;&#039;&#039; (better for many reasons) &amp;lt;!-- to allow preview before downloading; important with slow connections, and also for easy access to the ADS page with the published version when coming back to this later --&amp;gt;&lt;br /&gt;
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other)&lt;br /&gt;
* Within a subject, maybe sort by descending chronological order, to have the newest on top; no need to put a date since the month+year is in the arXiv link (shown when hovering over it)&lt;br /&gt;
* Comments+discussions go onto the page [[Talk:Papers|Discussion]].&lt;br /&gt;
&lt;br /&gt;
Enjoy reading!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
* Young, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs == &lt;br /&gt;
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184, &amp;quot;The influence of accretion bursts on methanol and water in massive young stellar objects&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882, &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating&amp;quot;&lt;br /&gt;
&lt;br /&gt;
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 &amp;quot;Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 &amp;quot;State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other ==&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=User_talk:Vardan&amp;diff=47</id>
		<title>User talk:Vardan</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=User_talk:Vardan&amp;diff=47"/>
		<updated>2023-12-12T19:37:50Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Hi Vardan, just to test whether you get emails through this. -- Lothar&lt;br /&gt;
&lt;br /&gt;
Hi Lothar, yes, just got an email that you created this page. -- Vardan&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=44</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=44"/>
		<updated>2023-12-12T12:00:37Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Interesting papers can be put here. It would be useful to:&lt;br /&gt;
* Put the title and maybe author names&lt;br /&gt;
* Put a link to the abstract page, not to the PDF, to allow preview before downloading (very useful with slow connexions, and also for easy access to the ADS page with the published version when coming back to this later)&lt;br /&gt;
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other) instead of day, since the latter quickly becomes irrelevant&lt;br /&gt;
* Within a subject, maybe sort by descending chronological order, to have the newest on top&lt;br /&gt;
&lt;br /&gt;
I implemented this boldly---please review/improve this (maybe drop the division by topic since there will be ambiguous cases? or indicate the month?), &#039;&#039;&#039;delete this line&#039;&#039;&#039;, and delete the dates commented out in the Wiki source if they are not needed anymore. Danke!&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
&amp;lt;!-- === 07.12.23 === --&amp;gt;&lt;br /&gt;
* Young, [https://arxiv.org/abs/2312.03039 &amp;quot;Insights into the first and second hydrostatic core stages from numerical simulations&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 &amp;quot;Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Discs ==&lt;br /&gt;
&amp;lt;!-- === 08.12.23 === --&amp;gt;&lt;br /&gt;
* Higginbottom et al. 2023, [https://arxiv.org/abs/2312.06042 State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows]&lt;br /&gt;
&lt;br /&gt;
* Nixon et al., [https://arxiv.org/abs/2312.04400 &amp;quot;On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
* Stapper et al., [https://arxiv.org/abs/2312.03835 &amp;quot;Constraining the gas mass of Herbig disks using CO isotopologues&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- === 11.12.23 === --&amp;gt;&lt;br /&gt;
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 &amp;quot;High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- === 20.10.223 === --&amp;gt;&lt;br /&gt;
* Chen et al., [https://arxiv.org/abs/2310.13690 &amp;quot;Planet Gap-opening Feedback on Disk Thermal Structure and Composition&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
&amp;lt;!-- === 18.10.2023 === --&amp;gt;&lt;br /&gt;
* Cattolico &amp;amp; Perets, [https://arxiv.org/abs/2310.11583 &amp;quot;Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Planets ==&lt;br /&gt;
&amp;lt;!-- === 11.12.23 === --&amp;gt;&lt;br /&gt;
* Portegies Zwart &amp;amp; Hochart, [https://arxiv.org/abs/2312.04645 &amp;quot;The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Small things ==&lt;br /&gt;
&amp;lt;!-- === 05.12.23 === --&amp;gt;&lt;br /&gt;
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 &amp;quot;The bouncing barrier revisited: Impact on key planet formation processes and observational signatures&amp;quot;]&lt;br /&gt;
* Houge et al., [https://arxiv.org/abs/2312.01856 &amp;quot;Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles&amp;quot;]&lt;br /&gt;
&lt;br /&gt;
== Other ==&lt;br /&gt;
* Dib &amp;amp; Menou, [https://arxiv.org/abs/2312.02091 &amp;quot;Physics simulation capabilities of LLMs&amp;quot;]&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=41</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=41"/>
		<updated>2023-12-11T10:05:26Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Here is an interesting paper: https://arxiv.org/abs/2310.11583&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/abs/2310.13690 (interesting!)&lt;br /&gt;
&lt;br /&gt;
=== 05.12.23 ===&lt;br /&gt;
https://arxiv.org/abs/2312.01856&lt;br /&gt;
&lt;br /&gt;
=== 07.12.23 ===&lt;br /&gt;
https://arxiv.org/pdf/2312.03039.pdf&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/pdf/2312.03272.pdf&lt;br /&gt;
&lt;br /&gt;
=== 08.12.23 ===&lt;br /&gt;
https://arxiv.org/pdf/2312.04400.pdf&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/pdf/2312.03835.pdf&lt;br /&gt;
&lt;br /&gt;
=== 11.12.23 ===&lt;br /&gt;
https://arxiv.org/pdf/2312.04645.pdf&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/pdf/2312.04618.pdf&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=40</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=40"/>
		<updated>2023-12-08T10:09:39Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Here is an interesting paper: https://arxiv.org/abs/2310.11583&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/abs/2310.13690 (interesting!)&lt;br /&gt;
&lt;br /&gt;
=== 05.12.23 ===&lt;br /&gt;
https://arxiv.org/abs/2312.01856&lt;br /&gt;
&lt;br /&gt;
=== 07.12.23 ===&lt;br /&gt;
https://arxiv.org/pdf/2312.03039.pdf&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/pdf/2312.03272.pdf&lt;br /&gt;
&lt;br /&gt;
=== 08.12.23 ===&lt;br /&gt;
https://arxiv.org/pdf/2312.04400.pdf&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/pdf/2312.03835.pdf&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=39</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=39"/>
		<updated>2023-12-07T12:32:24Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Here is an interesting paper: https://arxiv.org/abs/2310.11583&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/abs/2310.13690 (interesting!)&lt;br /&gt;
&lt;br /&gt;
=== 05.12.23 ===&lt;br /&gt;
https://arxiv.org/abs/2312.01856&lt;br /&gt;
&lt;br /&gt;
=== 07.12.23 ===&lt;br /&gt;
https://arxiv.org/pdf/2312.03039.pdf&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/pdf/2312.03272.pdf&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
	<entry>
		<id>https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=38</id>
		<title>Papers</title>
		<link rel="alternate" type="text/html" href="https://wiki.uni-due.de/agk/index.php?title=Papers&amp;diff=38"/>
		<updated>2023-12-05T12:33:11Z</updated>

		<summary type="html">&lt;p&gt;Vardan: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Here is an interesting paper: https://arxiv.org/abs/2310.11583&lt;br /&gt;
&lt;br /&gt;
https://arxiv.org/abs/2310.13690 (interesting!)&lt;br /&gt;
&lt;br /&gt;
=== 05.12.23 ===&lt;br /&gt;
https://arxiv.org/abs/2312.01856&lt;/div&gt;</summary>
		<author><name>Vardan</name></author>
	</entry>
</feed>