Evolution of galaxy cluster scaling from XMM-Newton observation of the galaxy clusters at z ⩾ 0.4
Abstract
We present here new XMM-Newton observations of 3 relatively cool clusters at z ≈ 0.4, complemented by archival observations of 3 other clusters at similar redshift. We derived the M- T and R- T relations from the hydrostatic equation using an isothermal temperature distribution.
- Publication:
-
Advances in Space Research
- Pub Date:
- August 2008
- DOI:
- 10.1016/j.asr.2008.03.008
- Bibcode:
- 2008AdSpR..42..576A
