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| | [[File:Pair_stage.png|300px|center| galaxy pair merging stage(2020ApJ...892L..20F)]] | ||
===Compact groups of galaxies === | ===Compact groups of galaxies === | ||
*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.jpg|200px|thumb| | [[File:CG.jpg|200px|thumb|center| compact groups of galaxies(2020ApJS..246...12Z)]] | ||
===Dust geometry of galaxies === | ===Dust geometry of galaxies === | ||
*How to measure or quantify the geometry of the dust components? | *How to measure or quantify the geometry of the dust components? | ||
*How the dust geometries affect the observed properties of galaxies? | *How the dust geometries affect the observed properties of galaxies? | ||
[[File:图片1.png|200px|thumb| | [[File:图片1.png|200px|thumb|center| dust geometry model of disk galaxies]] | ||
===HII regions of galaxies === | ===HII regions of galaxies === | ||
*Identify HII regions in local star-forming galaxies using MaNGA data | *Identify HII regions in local star-forming galaxies using MaNGA data | ||
* Characterize the star formation process of HII regions | * Characterize the star formation process of HII regions | ||
[[File:HII.png| | [[File:HII.png|300px|thumb|center| HII regions identified from MaNGA maps]] | ||
==Zheng Zhenya == | ==Zheng Zhenya == | ||
Revision as of 07:49, 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
- ---