Difference between revisions of "SHAO-KIAA galaxies"

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== large scale structure of galaxy distribution (Guo Hong)==
== Guo Hong==
* large scale structure of galaxy distribution
* ---


==ionized gas of galaxies (Hao Lei) ==
==Hao Lei ==
* ionized gas of galaxies  
* ---


==structure of galaxies(Shen Shiyin)==
==Shen Shiyin==
[[File:Shiyin.jpg|thumb |shiyin]]
[[File:Shiyin.jpg|thumb |shiyin]]
*Dust geometry of galaxies
* 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 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|thumb dust geometry]]
[[File:图片1.png|thumb dust geometry]]


 
* 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|thumb HII regions]]
[[File:HII.png|thumb HII regions]]


==high redshift galaxies (Zheng Zhenya) ==
==Zheng Zhenya ==
* high redshift galaxies
* ---


==galactic dynamics (Zhu Lin) ==
==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.
* galactic dynamics
* ---

Revision as of 07:27, 24 June 2020

Guo Hong

  • large scale structure of galaxy distribution
  • ---

Hao Lei

  • ionized gas of galaxies
  • ---

Shen Shiyin

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?

thumb dust geometry

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

thumb HII regions

Zheng Zhenya

  • high redshift galaxies
  • ---

Zhu Lin

  • galactic dynamics
  • ---