Difference between revisions of "SHAO-KIAA galaxies"
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* Galaxy pair and galaxy interaction | * Galaxy pair and galaxy interaction | ||
: How to quantify the merging stage of galaxies | : How to quantify the merging stage of galaxies? | ||
[[File:Pair_stage.png|400px| galaxy pair merging stage]] | [[File:Pair_stage.png|400px| galaxy pair merging stage]] | ||
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: the largest and most complete low redshift compact groups of galaxies(CGs) sample selected from SDSS and LAMOST | : the largest and most complete low redshift compact groups of galaxies(CGs) sample selected from SDSS and LAMOST | ||
: Dynamics and physical nature CGs | : Dynamics and physical nature CGs | ||
[[File:CG.png|400px| compact groups of galaxies]] | |||
* Dust geometry of galaxies | * Dust geometry of galaxies | ||
Revision as of 07:38, 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
- ---