Papers: Difference between revisions
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== Stars == | == 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”"] | * 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"] | * Young 2023, [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"] | * 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 == | == Discs == | ||
* Fenton & Stamatellos 2024, [https://arxiv.org/ | * 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"] | * 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"] | ||
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== Planets == | == 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"] | * Krapp et al. 2024, [https://arxiv.org/abs/2402.14638 "A thermodynamic criterion for the formation of Circumplanetary Disks"] | ||
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* Burn et al. 2024, [https://arxiv.org/abs/2401.04380 "A radius valley between migrated steam worlds and evaporated rocky cores"] | * 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/ | * 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/ | * 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 == | ||
* Birnstiel 2023, [https://arxiv.org/abs/2312.13287 "Dust growth and evolution in protoplanetary disks"] | * Birnstiel 2023, [https://arxiv.org/abs/2312.13287 "Dust growth and evolution in protoplanetary disks"] | ||
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* 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"] | * 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
- Balmer et al. 2023, "VLTI/GRAVITY Provides Evidence the Young, Substellar Companion HD 136164 Ab formed like a “Failed Star”"
- López-Vázquez et al. 2023, "Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow"
- Usmanov et al. 2012, "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, "Time-dependent long-term hydrodynamic simulations of the inner protoplanetary disk III: The influence of photoevaporation"
- Fenton & Stamatellos 2024, "The 3D structure of disc-instability protoplanets"
- Takakuwa et al. 2024, "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, "A Companion in V1247 Ori Supported by Spiral Arm Pattern Motion"
- Jiang et al. 2023, "Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks"
- Ashraf et al. 2023, "An outburst and FU Ori-type disk of a former low luminosity protostar"
- Guadarrama et al. 2023, "The influence of accretion bursts on methanol and water in massive young stellar objects"
- Fuksman et al. 2023, "Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks I. Angular momentum transport and turbulent heating"
- Fuksman et al. 2023, "Vertical shear instability in two-moment radiation-hydrodynamical simulations of irradiated protoplanetary disks II. Secondary instabilities and stability regions"
- Higginbottom et al., "State-of-the-art simulations of line-driven accretion disc winds: realistic radiation-hydrodynamics leads to weaker outflows"
- Nixon et al., "On the role of numerical diffusivity in MHD simulations of global accretion disc dynamos"
- Paneque-Carreño et al., "High turbulence in the IM Lup protoplanetary disk: Direct observational constraints from CN and C_2H emission"
- Cattolico & Perets, "Dynamical evolution of second-generation circumstellar/protoplanetary disks in evolved wide binary systems"
Planets
- Lega et al. 2024, "Gas dynamics around a Jupiter-mass planet I. Influence of protoplanetary disk properties"
- Zhang 2024, "Initial Entropy and Potential Delayed Formation of the Directly Imaged Exoplanet AF Lep b"
- Savignac & Lee 2024, "The Not-So Dramatic Effect of Advective Flows on Gas Accretion"
- Krapp et al. 2024, "A thermodynamic criterion for the formation of Circumplanetary Disks"
- Andama et al. 2024, "What stars can form planets: planetesimal formation at low"
- Lorek & Johansen 2024, "Formation of flattened planetesimals by gravitational collapse of rotating pebble clouds"
- Jones et al. 2024, "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, "Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures"
- Portegies Zwart & Hochart, "The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters"
Small things
- Birnstiel 2023, "Dust growth and evolution in protoplanetary disks"
- Dominik and Dullemond 2023, "The bouncing barrier revisited: Impact on key planet formation processes and observational signatures"
Other (including ornithology)
- Van Wassenbergh & Mielke (2024), "Why woodpeckers don’t get concussions", Physics Today (short read)
- Dib & Menou, "Physics simulation capabilities of LLMs"
- Keto (2020), "Stability and solution of the time-dependent Bondi–Parker flow"
- Bratley & Fox (1988), "Algorithm 659: Implementing Sobol's quasirandom sequence generator"
- Smith (1987), "A note on the Stokes paradox"
- Davis (1959), "Leonhard Euler's Integral: A Historical Profile of the Gamma Function"