Galaxy stellar mass functions of different morphological types in clusters, and their evolution between z= 0.8 and 0
We present the galaxy stellar mass function and its evolution in clusters from z˜ 0.8 to the current epoch, based on the WIde-field Nearby Galaxy-cluster Survey (WINGS) (0.04 ≤z≤ 0.07), and the ESO Distant Cluster Survey (EDisCS) (0.4 ≤z≤ 0.8). We investigate the total mass function and find that it evolves noticeably with redshift. The shape at M*
Vulcani, Benedetta et al.
Fecha de publicación:
3
2011