Evolution of galaxy cluster scaling from XMM-Newton observation of the galaxy clusters at z ⩾ 0.4

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Scientific paper

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.

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