“SHAO-KIAA galaxies”的版本间差异
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== Guo Hong== |
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* large scale structure of galaxy distribution |
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==Hao Lei == |
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==Shen Shiyin== |
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[[File:Shiyin.jpg|thumb |
[[File:Shiyin.jpg|200px|thumb shiyin]] |
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===Galaxy pair and galaxy interaction=== |
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* How to quantify the merging stage of galaxy pairs? Kinemetry, Morphlogy? |
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* Physical process in different stages? |
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[[File:Pair_stage.png|300px|thumb|center| galaxy pair merging stage(2020ApJ...892L..20F)]] |
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===Compact groups of galaxies === |
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*the largest and most complete low redshift compact groups of galaxies(CGs) sample selected from SDSS and LAMOST. |
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*Dynamics and physical nature CGs? |
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[[File:CG.jpg|300px|thumb|center| compact groups of galaxies in SDSS+LAMOST (2020ApJS..246...12Z)]] |
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===Dust geometry of galaxies === |
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===HII regions of galaxies === |
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==Zheng Zhenya == |
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We probe the mass distributions, e.g. dark matter distribution, black hole mass in the inner regions of galaxies, by modelling the motion of particles. On the other hand, the motion of particles itself, that is their orbit distribution, can tell us the galaxies' assembly history. |
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===Epoch of Reionization (EoR)=== |
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* How to probe EoR via galaxies? |
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* 21cm & Ly-α in EoR |
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===High-Redshift Galaxies=== |
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* Physical properties of high-redshift galaxies |
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* Evolution of high-redshift galaxies |
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* Galaxy protoclusters at high-redshift |
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==Zhu Lin == |
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* --- |
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2020年6月24日 (三) 08:39的最新版本
Guo Hong
- large scale structure of galaxy distribution
- ---
Hao Lei
- ionized gas of galaxies
- ---
Shen Shiyin
Galaxy pair and galaxy interaction
- How to quantify the merging stage of galaxy pairs? Kinemetry, Morphlogy?
- Physical process in different stages?
Compact groups of galaxies
- the largest and most complete low redshift compact groups of galaxies(CGs) sample selected from SDSS and LAMOST.
- Dynamics and physical nature CGs?
Dust geometry of galaxies
- How to measure or quantify the geometry of the dust components?
- How the dust geometries affect the observed properties of galaxies?
HII regions of galaxies
- Identify HII regions in local star-forming galaxies using MaNGA data.
- Characterize the star formation process of HII regions.
Zheng Zhenya
Epoch of Reionization (EoR)
- How to probe EoR via galaxies?
- 21cm & Ly-α in EoR
High-Redshift Galaxies
- Physical properties of high-redshift galaxies
- Evolution of high-redshift galaxies
- Galaxy protoclusters at high-redshift
Zhu Lin
- galactic dynamics
- ---