“SHAO-KIAA galaxies”的版本间差异

2020年6月24日 (三) 07:49的版本

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)

dust geometry model of disk galaxies

HII regions identified from MaNGA maps

@@ 第13行： / 第13行： @@
 ===Galaxy pair and galaxy interaction===
 * How to quantify the merging stage of galaxies?
-[[File:Pair_stage.png|200px|left|  galaxy pair merging stage(2020ApJ...892L..20F)]]
+[[File:Pair_stage.png|300px|center|  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|200px|thumb|left| compact groups of galaxies(2020ApJS..246...12Z)]]
+[[File:CG.jpg|200px|thumb|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?
-[[File:图片1.png|200px|thumb|left| dust geometry model of disk galaxies]]
+[[File:图片1.png|200px|thumb|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
-[[File:HII.png|200px|thumb|left| HII regions identified from MaNGA maps]]
+[[File:HII.png|300px|thumb|center| HII regions identified from MaNGA maps]]
 ==Zheng Zhenya ==