Papers: Difference between revisions
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Interesting papers can be put here. | 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 | * 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) | * Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other) | ||
* Within a subject, maybe sort by descending chronological order, to have the newest on top | * 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) | ||
Enjoy reading! | |||
== Stars == | == Stars == | ||
* Young, [https://arxiv.org/abs/2312.03039 "Insights into the first and second hydrostatic core stages from numerical simulations"] | * Young, [https://arxiv.org/abs/2312.03039 "Insights into the first and second hydrostatic core stages from numerical simulations"] | ||
| Line 14: | Line 13: | ||
== Discs == | == Discs == | ||
* 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"] | |||
* Higginbottom et al. | |||
* 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"] | ||
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* 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"] | ||
* 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"] | ||
* 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"] | ||
* 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 == | ||
* 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 == | ||
* Dominik and Dullemond 2023, [https://arxiv.org/abs/2312.06000 "The bouncing barrier revisited: Impact on key planet formation processes and observational signatures"] | * 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 == | ||
* 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"] | ||
Revision as of 19:11, 12 December 2023
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)
- Maybe sort by subject (e.g.: Stars, Discs, Planets, Dust/rocks/pebbles, Other)
- 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)
Enjoy reading!
Stars
- López-Vázquez et al., "Multiple shells driven by disk winds: ALMA observations in the HH 30 outflow"
Discs
- 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
- Portegies Zwart & Hochart, "The origin and evolution of wide Jupiter Mass Binary Objects in young stellar clusters"
Small things
- Dominik and Dullemond 2023, "The bouncing barrier revisited: Impact on key planet formation processes and observational signatures"
Other
- Dib & Menou, "Physics simulation capabilities of LLMs"