“SHAO-KIAA galaxies”的版本间差异

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==Shen Shiyin==
==Shen Shiyin==
[[File:Shiyin.jpg|200px|thumb|right| shiyin]]
[[File:Shiyin.jpg|200px|thumb shiyin]]




* Galaxy pair and galaxy interaction
===Galaxy pair and galaxy interaction===
: How to quantify the merging stage of galaxies
* How to quantify the merging stage of galaxy pairs? Kinemetry, Morphlogy?
* Physical process in different stages?
: [[File:Pair_stage.png|400px|thumb|left galaxy pair merging stage]]
[[File:Pair_stage.png|300px|thumb|center| galaxy pair merging stage(2020ApJ...892L..20F)]]


* 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)]]


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===Dust geometry of galaxies ===
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*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?
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[[File:图片1.png|300px|thumb|center| dust geometry model of disk galaxies]]


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===HII regions of galaxies ===
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*Identify HII regions in local star-forming galaxies using MaNGA data.
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* Characterize the star formation process of HII regions.
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[[File:HII.png|300px|thumb|center| HII regions identified from MaNGA maps]]


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==Zheng Zhenya ==
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* 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?
⚫
[[File:图片1.png|thumb dust geometry]]


===Epoch of Reionization (EoR)===
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* HII regions of galaxies
* How to probe EoR via galaxies?
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:Identify HII regions in local star-forming galaxies using MaNGA data
* 21cm & Ly-α in EoR
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:Characterize the star formation process of HII regions
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[[File:HII.png|thumb HII regions]]


===High-Redshift Galaxies===
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==Zheng Zhenya ==
* high redshift galaxies
* Physical properties of high-redshift galaxies
* Evolution of high-redshift galaxies
* ---
* Galaxy protoclusters at high-redshift


==Zhu Lin ==
==Zhu Lin ==

2020年6月24日 (三) 08:39的最新版本

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 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

Epoch of Reionization (EoR)

  • How to probe EoR via galaxies?
  • 21cm & Ly-α in EoR

High-Redshift Galaxies

  • Physical properties of high-redshift galaxies
  • Evolution of high-redshift galaxies
  • Galaxy protoclusters at high-redshift

Zhu Lin

  • galactic dynamics
  • ---
取自“http://cluster.shao.ac.cn/wiki/index.php?title=SHAO-KIAA_galaxies&oldid=3760”