“SHAO-KIAA galaxies”的版本间差异
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无编辑摘要 |
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== Guo Hong== |
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* large scale structure of galaxy distribution |
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* --- |
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==Hao Lei == |
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* --- |
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==Shen Shiyin== |
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[[File:Shiyin.jpg|thumb |shiyin]] |
[[File:Shiyin.jpg|thumb |shiyin]] |
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* Galaxy pair and galaxy interaction |
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: How to quantify the merging stage of galaxies |
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* Compact groups of galaxies |
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: 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 |
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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|thumb dust geometry]] |
[[File:图片1.png|thumb dust geometry]] |
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* HII regions of galaxies |
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:Identify HII regions in local star-forming galaxies using MaNGA data |
:Identify HII regions in local star-forming galaxies using MaNGA data |
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:Characterize the star formation process of HII regions |
:Characterize the star formation process of HII regions |
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[[File:HII.png|thumb HII regions]] |
[[File:HII.png|thumb HII regions]] |
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==Zheng Zhenya == |
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* high redshift galaxies |
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* --- |
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==Zhu Lin == |
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* galactic dynamics |
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We probe the mass distributions, e.g. dark matter distribution, black hole mass in the inner regions of galaxies, by modelling the motion of particles. On the other hand, the motion of particles itself, that is their orbit distribution, can tell us the galaxies' assembly history. |
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* --- |
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2020年6月24日 (三) 07:27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
- ---