SHAO-KIAA galaxies

From cluster
Revision as of 07:00, 24 June 2020 by Shen (talk | contribs) (Created page with "== large scale structure of galaxy distribution (Guo Hong)== ==ionized gas of galaxies (Hao Lei) == ==structure of galaxies(Shen Shiyin)== ==high redshift galaxies (Zheng Z...")
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
Jump to navigation Jump to search

large scale structure of galaxy distribution (Guo Hong)

ionized gas of galaxies (Hao Lei)

structure of galaxies(Shen Shiyin)

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.