“SHAO-KIAA galaxies”的版本间差异
跳到导航
跳到搜索
第13行: | 第13行: | ||
===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|300px|center| galaxy pair merging stage(2020ApJ...892L..20F)]] |
[[File:Pair_stage.png|300px|thumb|center| galaxy pair merging stage(2020ApJ...892L..20F)]] |
||
===Compact groups of galaxies === |
===Compact groups of galaxies === |
2020年6月24日 (三) 07:50的版本
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 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
- ---