“SHAO-KIAA galaxies”的版本间差异
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===Galaxy pair and galaxy interaction=== |
===Galaxy pair and galaxy interaction=== |
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* How to quantify the merging stage of galaxy pairs? Kinemetry, Morphlogy? |
* How to quantify the merging stage of galaxy pairs? Kinemetry, Morphlogy? |
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* Physical process in different stages |
* Physical process in different stages |
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[[File:Pair_stage.png|300px|thumb|center| galaxy pair merging stage(2020ApJ...892L..20F)]] |
[[File:Pair_stage.png|300px|thumb|center| galaxy pair merging stage(2020ApJ...892L..20F)]] |
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2020年6月24日 (三) 07:56的版本
Guo Hong
- large scale structure of galaxy distribution
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Hao Lei
- ionized gas of galaxies
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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
- high redshift galaxies
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Zhu Lin
- galactic dynamics
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