“SHAO-KIAA galaxies”的版本间差异

2020年6月24日 (三) 07:44的版本

How to quantify the merging stage 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(2020ApJS..246...12Z)

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

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

@@ 第14行： / 第14行： @@
 : How to quantify the merging stage of galaxies?
-[[File:Pair_stage.png|400px|right|  galaxy pair merging stage(2020ApJ...892L..20F)]]
+[[File:Pair_stage.png|200px|right|  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
-[[File:CG.jpg|400px|thumb| compact groups of galaxies(2020ApJS..246...12Z)]]
+[[File:CG.jpg|200px|thumb| 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?
-[[File:图片1.png|400px | dust geometry]]
+[[File:图片1.png|200px|thumb|right| 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
-[[File:HII.png|400px | HII regions]]
+[[File:HII.png|200px|thumb|right| HII regions identified from MaNGA maps]]
 ==Zheng Zhenya ==