Evolution of galaxy cluster scaling and structural properties from XMM observations: probing the physics of structure formation
Abstract
We will present a study of two low luminosity distant clusters of galaxies z 0 4-0 5 observed with XMM-Newton Their properties will be compared to that of massive distant clusters those of nearby clusters similar mass This will be discussed in the framework of the self-similarity model of cluster formation
- Publication:
-
36th COSPAR Scientific Assembly
- Pub Date:
- 2006
- Bibcode:
- 2006cosp...36..558A