“SHAO-KIAA galaxies”的版本间差异
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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:HII.png|thumb|dust geometry]] |
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*HII regions of galaxies |
*HII regions of galaxies |
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2020年6月24日 (三) 07:11的版本
large scale structure of galaxy distribution (Guo Hong)
ionized gas of galaxies (Hao Lei)
structure of galaxies(Shen Shiyin)
- 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
high redshift galaxies (Zheng Zhenya)
galactic dynamics （Zhu Lin)
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.