Evolution of galaxy cluster scaling from XMM-Newton observation of the galaxy clusters at z ⩾ 0.4
DOI: 10.1016/j.asr.2008.03.008
Bibcode: 2008AdSpR..42..576A
Anokhin, S. G.
France
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.
2008
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Advances in Space Research
XMM-Newton
1