“SHAO-KIAA galaxies”的版本间差异
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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 |
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*Dynamics and physical nature CGs |
*Dynamics and physical nature CGs |
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[[File:CG.jpg|200px|thumb|center compact groups of galaxies(2020ApJS..246...12Z)]] |
[[File:CG.jpg|200px|thumb|center| compact groups of galaxies(2020ApJS..246...12Z)]] |
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===Dust geometry of galaxies === |
===Dust geometry of galaxies === |
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*How to measure or quantify the geometry of the dust components? |
*How to measure or quantify the geometry of the dust components? |
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*How the dust geometries affect the observed properties of galaxies? |
*How the dust geometries affect the observed properties of galaxies? |
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[[File:图片1.png|200px|thumb|center dust geometry model of disk galaxies]] |
[[File:图片1.png|200px|thumb|center| dust geometry model of disk galaxies]] |
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===HII regions of galaxies === |
===HII regions of galaxies === |
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2020年6月24日 (三) 07:48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 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
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Zhu Lin
- galactic dynamics
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