SHAO-KIAA galaxies: Difference between revisions
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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| |
[[File:图片1.png|400px | dust geometry]] |
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* HII regions of galaxies |
* 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| |
[[File:HII.png|400px | HII regions]] |
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==Zheng Zhenya == |
==Zheng Zhenya == |
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Revision as of 07:35, 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
- ---