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Evolution of galaxy cluster scaling from XMM-Newton observation of the galaxy clusters at z ⩾ 0.4
Authors:SG Anokhin
Institution:CEA/DSM/DAPNIA, Service d’Astrophysique, L’Orme des Merisiers, Bât. 709, 91191 Gif-Sur-Yvette, 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 MT and RT relations from the hydrostatic equation using an isothermal temperature distribution.
Keywords:Galaxies clusters  X-ray astronomy  Scaling relations
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