Papers: Difference between revisions

From Arbeitsgruppe Kuiper
Jump to navigation Jump to search
(Änderungen an der Struktur!)
 
(35 intermediate revisions by 3 users not shown)
Line 1: Line 1:
Interesting papers can be put here. It would be useful to:
Interesting papers can be put here. Please:
* Put the title and maybe author names
* Indicate the title and some author information
* 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)
* Put a link to the '''abstract page, not to the PDF''' (better for many reasons) <!-- 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 -->
* Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other) instead of day, since the latter quickly becomes irrelevant
* Within a subject, sort by descending chronological order of addition (i.e., newest on top)
* Within a subject, maybe sort by descending chronological order, to have the newest on top
* Put comments and discussions on the page [[Talk:Papers|Discussion]].


I implemented this boldly---feel free to review/improve this, '''delete this line''', and delete the "date comments" in the source. Danke!
Enjoy reading!


== Stars ==
== Stars ==
<!-- === 07.12.23 === -->
* Young, [https://arxiv.org/abs/2312.03039 "Insights into the first and second hydrostatic core stages from numerical simulations"]


* López-Vázquez et al., [https://arxiv.org/abs/2312.03272 "Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow"]
* 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”"]
 
* Young 2023, [https://arxiv.org/abs/2312.03039 "Insights into the first and second hydrostatic core stages from numerical simulations"]
 
* López-Vázquez et al. 2023, [https://arxiv.org/abs/2312.03272 "Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow"]
 
* Usmanov et al. 2012, [https://iopscience.iop.org/article/10.1088/0004-637X/754/1/40 "Three-Dimensional Magnetohydrodynamic Modeling of the Solar Wind Including Pickup Protons and Turbulence Transport"] (superimposed grids to avoid the coordinate singularity at the poles)
 
== Discs ==
 
* Cecil, Gehrig & Steiner 2024, [https://arxiv.org/abs/2405.05816 "Time-dependent long-term hydrodynamic simulations of the inner protoplanetary disk III: The influence of photoevaporation"]
 
* Fenton & Stamatellos 2024, [https://arxiv.org/abs/2402.01432 "The 3D structure of disc-instability protoplanets"]
 
* Takakuwa et al. 2024, [https://arxiv.org/abs/2401.08722 "Early Planet Formation in Embedded Disks (eDisk) XIV: Flared Dust Distribution and Viscous Accretion Heating of the Disk around R CrA IRS 7B-a"]
 
* Ren et al. 2024, [https://arxiv.org/abs/2310.15430 "A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion"]
 
* Lim et al 2023, [https://arxiv.org/abs/2312.12508 "Streaming Instability and Turbulence: Conditions for Planetesimal Formation"]
 
* Jiang et al. 2023, [https://ui.adsabs.harvard.edu/abs/2023A%2526A...678A..33J "Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks"]
 
* Ashraf et al. 2023, [https://arxiv.org/abs/2312.10827 "An outburst and FU Ori-type disk of a former low luminosity protostar"]
 
* Guadarrama et al. 2023, [https://arxiv.org/abs/2312.07184 "The influence of accretion bursts on methanol and water in massive young stellar objects"]
 
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06882 "Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating"]
 
* Fuksman et al. 2023, [https://arxiv.org/abs/2312.06890 "Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions"]
 
* Higginbottom et al., [https://arxiv.org/abs/2312.06042 "State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows"]


== Discs ==
<!-- === 08.12.23 === -->
* Nixon et al., [https://arxiv.org/abs/2312.04400 "On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos"]
* Nixon et al., [https://arxiv.org/abs/2312.04400 "On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos"]


* Stapper et al., [https://arxiv.org/abs/2312.03835 "Constraining the gas mass of Herbig disks using CO isotopologues"]
* Stapper et al., [https://arxiv.org/abs/2312.03835 "Constraining the gas mass of Herbig disks using CO isotopologues"]


<!-- === 11.12.23 === -->
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 "High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission"]
* Paneque-Carreño et al., [https://arxiv.org/abs/2312.04618 "High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission"]


<!-- === 20.10.223 === -->
* Chen et al., [https://arxiv.org/abs/2310.13690 "Planet Gap-opening Feedback on Disk Thermal Structure and Composition"]
* Chen et al., [https://arxiv.org/abs/2310.13690 "Planet Gap-opening Feedback on Disk Thermal Structure and Composition"]


<!-- === 18.10.2023 === -->
* Cattolico & Perets, [https://arxiv.org/abs/2310.11583 "Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems"]
* Cattolico & Perets, [https://arxiv.org/abs/2310.11583 "Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems"]


== Planets ==
== Planets ==
<!-- === 11.12.23 === -->
 
* Lega et al. 2024, [https://arxiv.org/abs/2408.12233 "Gas dynamics around a Jupiter-mass planet I. Influence of protoplanetary disk properties"]
 
* Zhang 2024, [https://iopscience.iop.org/article/10.3847/2515-5172/ad4481 "Initial Entropy and Potential Delayed Formation of the Directly Imaged Exoplanet AF Lep b"]
 
* Savignac & Lee 2024, [https://arxiv.org/abs/2310.06013 "The Not-So Dramatic Effect of Advective Flows on Gas Accretion"]
 
* Krapp et al. 2024, [https://arxiv.org/abs/2402.14638 "A thermodynamic criterion for the formation of Circumplanetary Disks"]
 
* Andama et al. 2024, [https://arxiv.org/abs/2401.16155 "What stars can form planets: planetesimal formation at low"]
 
* Law et al. 2024, [https://arxiv.org/abs/2401.03018 "Mapping the Vertical Gas Structure of the Planet-hosting PDS 70 Disk"]
 
* Lorek & Johansen 2024, [https://arxiv.org/abs/2401.05101 "Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds"]
 
* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 "A radius valley between migrated steam worlds and evaporated rocky cores"]
 
* Jones et al. 2024, [https://arxiv.org/abs/2401.09657 "A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS"]
 
* Xu & Wang 2024, [https://arxiv.org/abs/2401.06217 "Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures"]
 
* Portegies Zwart & Hochart, [https://arxiv.org/abs/2312.04645 "The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters"]
* Portegies Zwart & Hochart, [https://arxiv.org/abs/2312.04645 "The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters"]


== Small things ==
== Small things ==
<!-- === 05.12.23 === -->
 
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 "Dust growth and evolution in protoplanetary disks"]
 
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 "The bouncing barrier revisited: Impact on key planet formation processes and observational signatures"]
 
* Houge et al., [https://arxiv.org/abs/2312.01856 "Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles"]
* Houge et al., [https://arxiv.org/abs/2312.01856 "Surviving the Heat: multi-wavelength analysis of V883 Ori reveals that dust aggregates survive the sublimation of their ice mantles"]


== Other ==
== Other (including ornithology) ==
 
* Van Wassenbergh & Mielke (2024), [https://doi.org/10.1063/PT.3.5385 "Why woodpeckers don’t get concussions"], Physics Today (''short read'')
* Dib & Menou, [https://arxiv.org/abs/2312.02091 "Physics simulation capabilities of LLMs"]
* Dib & Menou, [https://arxiv.org/abs/2312.02091 "Physics simulation capabilities of LLMs"]
* Keto (2020), [https://doi.org/10.1093/mnras/staa529 "Stability and solution of the time-dependent Bondi–Parker flow"]
* Bratley & Fox (1988), [https://doi.org/10.1145/42288.214372 "Algorithm 659: Implementing Sobol's quasirandom sequence generator"]
* Smith (1987), [https://doi.org/10.1090/QAM%2F910459 "A note on the Stokes paradox"]
* Davis (1959), [https://doi.org/10.1080/00029890.1959.11989422 "Leonhard Euler's Integral: A Historical Profile of the Gamma Function"]

Latest revision as of 09:01, 23 August 2024

Interesting papers can be put here. Please:

  • Indicate the title and some author information
  • Put a link to the abstract page, not to the PDF (better for many reasons)
  • Within a subject, sort by descending chronological order of addition (i.e., newest on top)
  • Put comments and discussions on the page Discussion.

Enjoy reading!

Stars

Discs

Planets

Small things

Other (including ornithology)

Retrieved from "https://wiki.uni-due.de/agk/index.php?title=Papers&oldid=657"