wiki:arxiv
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wiki:arxiv [2022/06/09 07:35] Cheng Li |
wiki:arxiv [2023/12/04 22:19] (current) Cheng Li |
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| * [[https://arxiv.org/abs/2206.01548|Dust Formation in Astrophysical Environments: The Importance of Kinetics]] | * [[https://arxiv.org/abs/2206.01548|Dust Formation in Astrophysical Environments: The Importance of Kinetics]] | ||
| * [[https://arxiv.org/abs/2206.03510|ALPINE: A Large Survey to Understand Teenage Galaxies]] | * [[https://arxiv.org/abs/2206.03510|ALPINE: A Large Survey to Understand Teenage Galaxies]] | ||
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| + | ===== 2023 ===== | ||
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| ===== 2022 ===== | ===== 2022 ===== | ||
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| + | ==== July ==== | ||
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| + | * [[https://arxiv.org/abs/2207.05093|Turbulent Cold Flows Gave Birth to the First Quasars]] | ||
| ==== June ==== | ==== June ==== | ||
| + | * [[https://arxiv.org/abs/2206.04521|The stellar halo in Local Group Hestia simulations I. The in-situ component and the effect of mergers]] | ||
| + | * [[https://arxiv.org/abs/2206.04522|The stellar halo in Local Group Hestia simulations II. The accreted component]] | ||
| * [[https://arxiv.org/abs/2206.00681|Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies]] | * [[https://arxiv.org/abs/2206.00681|Pressure-Regulated, Feedback-Modulated Star Formation In Disk Galaxies]] | ||
| * [[https://arxiv.org/abs/2206.00662|The Size-Mass Relation of Post-Starburst Galaxies in the Local Universe]]: post-starburst galaxies in SDSS are found to be smaller than quiescent galaxies of same masses. I'm wondering whether the same effect is seen also in the MaNGA-based sample. | * [[https://arxiv.org/abs/2206.00662|The Size-Mass Relation of Post-Starburst Galaxies in the Local Universe]]: post-starburst galaxies in SDSS are found to be smaller than quiescent galaxies of same masses. I'm wondering whether the same effect is seen also in the MaNGA-based sample. | ||
wiki/arxiv.1654760121.txt.gz ยท Last modified: 2022/06/09 07:35 by Cheng Li
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