Difference between revisions of "SHAO-KIAA galaxies"

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===Compact groups of galaxies ===
===Compact groups of galaxies ===
*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.
*Dynamics and physical nature CGs
*Dynamics and physical nature CGs?
[[File:CG.jpg|300px|thumb|center| compact groups of galaxies in SDSS+LAMOST (2020ApJS..246...12Z)]]
[[File:CG.jpg|300px|thumb|center| compact groups of galaxies in SDSS+LAMOST (2020ApJS..246...12Z)]]



Revision as of 07:57, 24 June 2020

Guo Hong

  • large scale structure of galaxy distribution
  • ---

Hao Lei

  • ionized gas of galaxies
  • ---

Shen Shiyin

thumb shiyin


Galaxy pair and galaxy interaction

  • How to quantify the merging stage of galaxy pairs? Kinemetry, Morphlogy?
  • Physical process in different stages
galaxy pair merging stage(2020ApJ...892L..20F)

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?
compact groups of galaxies in SDSS+LAMOST (2020ApJS..246...12Z)

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?
dust geometry model of disk galaxies

HII regions of galaxies

  • Identify HII regions in local star-forming galaxies using MaNGA data
  • Characterize the star formation process of HII regions
HII regions identified from MaNGA maps

Zheng Zhenya

  • high redshift galaxies
  • ---

Zhu Lin

  • galactic dynamics
  • ---