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Here is an interesting paper: https://arxiv.org/abs/2310.11583
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) <!-- 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 -->
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https://arxiv.org/abs/2310.13690
Enjoy reading!
 
== Stars ==
 
* 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"]
 
* 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"]
 
* 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"]
 
* Chen et al., [https://arxiv.org/abs/2310.13690 "Planet Gap-opening Feedback on Disk Thermal Structure and Composition"]
 
* Cattolico & Perets, [https://arxiv.org/abs/2310.11583 "Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems"]
 
== Planets ==
 
* 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"]
 
== Small things ==
 
* 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"]
 
== 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"]
* 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)

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