Papers - Revision history

Vardan: /* Planets */

2024-08-23T08:01:31Z

Planets

← Older revision		Revision as of 10:01, 23 August 2024
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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"]		* 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"]

Lothar.brendel: /* Stars */ +Usmanov '12

2024-07-12T15:35:30Z

Stars: +Usmanov '12

← Older revision		Revision as of 17:35, 12 July 2024
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	* 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 ==

Lothar.brendel: /* Other (including ornithology) */ +Davis '59

2024-05-19T10:06:20Z

Other (including ornithology): +Davis '59

← Older revision		Revision as of 12:06, 19 May 2024
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	* Bratley & Fox (1988), [https://doi.org/10.1145/42288.214372 "Algorithm 659: Implementing Sobol's quasirandom sequence generator"]		* 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"]		* 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"]

Gabriel: Zwei Artikel

2024-05-14T13:51:38Z

Zwei Artikel

← Older revision		Revision as of 15:51, 14 May 2024
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	== Discs ==		== Discs ==

	* Fenton & Stamatellos 2024, [https://arxiv.org/~~pdf~~/2402.01432~~.pdf~~ "The 3D structure of disc-instability protoplanets"]		* 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 ==

			* 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"]		* Savignac & Lee 2024, [https://arxiv.org/abs/2310.06013 "The Not-So Dramatic Effect of Advective Flows on Gas Accretion"]
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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/~~pdf~~/2401.09657~~.pdf~~ "A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS"]		* 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/~~pdf~~/2401.06217~~.pdf~~ "Earths are not Super-Earths, Saturns are not Jupiters: Imprints of pressure-bump planet formation on planetary architectures"]		* 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"]

Lothar.brendel: /* Other (including ornithology) */ +Stokes Paradox

2024-05-08T08:25:27Z

Other (including ornithology): +Stokes Paradox

← Older revision		Revision as of 10:25, 8 May 2024
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	* 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"]		* 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"]

Lothar.brendel: /* Other (including ornithology) */ +Bratley & Fox

2024-05-03T05:40:30Z

Other (including ornithology): +Bratley & Fox

← Older revision		Revision as of 07:40, 3 May 2024
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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"]

Gabriel: Planetenartikel

2024-04-19T19:43:07Z

Planetenartikel

← Older revision		Revision as of 21:43, 19 April 2024
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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”"]

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	== Planets ==		== Planets ==

			* 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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	== 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"]

Lothar.brendel: /* Other (including ornithology) */ q'marks

2024-03-11T16:07:55Z

Other (including ornithology): q'marks

← Older revision		Revision as of 18:07, 11 March 2024
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	* Van Wassenbergh & Mielke (2024), [https://doi.org/10.1063/PT.3.5385 "Why woodpeckers don’t get concussions"], Physics Today (''short read'')		* 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]		* Keto (2020), [https://doi.org/10.1093/mnras/staa529 "Stability and solution of the time-dependent Bondi–Parker flow"]

Lothar.brendel: /* Other (including ornithology) */ +Keto

2024-03-11T16:06:36Z

Other (including ornithology): +Keto

← Older revision		Revision as of 18:06, 11 March 2024
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	* Van Wassenbergh & Mielke (2024), [https://doi.org/10.1063/PT.3.5385 "Why woodpeckers don’t get concussions"], Physics Today (''short read'')		* 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]

Vardan: /* Planets */

2024-02-23T09:48:59Z

Planets

← Older revision		Revision as of 11:48, 23 February 2024
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	== Planets ==		== Planets ==
			* 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"]		* Andama et al. 2024, [https://arxiv.org/abs/2401.16155 "What stars can form planets: planetesimal formation at low"]