SHAO-KIAA galaxies: Difference between revisions
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===Galaxy pair and galaxy interaction=== |
===Galaxy pair and galaxy interaction=== |
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[[File:Pair_stage.png|200px|right| galaxy pair merging stage(2020ApJ...892L..20F)]] |
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* How to quantify the merging stage of galaxies? |
* How to quantify the merging stage of galaxies? |
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Revision as of 07:47, 24 June 2020
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 galaxies?
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
- ---
Zhu Lin
- galactic dynamics
- ---