“SHAO-KIAA galaxies”的版本间差异

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*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|100px|thumb| compact groups of galaxies(2020ApJS..246...12Z)]]
[[File:CG.jpg|200px|thumb|center compact groups of galaxies(2020ApJS..246...12Z)]]


===Dust geometry of galaxies ===
===Dust geometry of galaxies ===
*How to measure or quantify the geometry of the dust components?
*How to measure or quantify the geometry of the dust components?
*How the dust geometries affect the observed properties of galaxies?
*How the dust geometries affect the observed properties of galaxies?
[[File:图片1.png|100px|thumb|right| dust geometry model of disk galaxies]]
[[File:图片1.png|200px|thumb|center dust geometry model of disk galaxies]]


===HII regions of galaxies ===
===HII regions of galaxies ===
*Identify HII regions in local star-forming galaxies using MaNGA data
*Identify HII regions in local star-forming galaxies using MaNGA data
* Characterize the star formation process of HII regions
* Characterize the star formation process of HII regions
[[File:HII.png|100px|thumb|right| HII regions identified from MaNGA maps]]
[[File:HII.png|200px|thumb|center| HII regions identified from MaNGA maps]]


==Zheng Zhenya ==
==Zheng Zhenya ==

2020年6月24日 (三) 07:48的版本

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 galaxies?
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
center compact groups of galaxies(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?
center 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
  • ---
取自“http://cluster.shao.ac.cn/wiki/index.php?title=SHAO-KIAA_galaxies&oldid=3746”