Abstract:We present the XMM-Newton X-ray analysis of 19 X-ray luminous galaxy clusters of low-to-mid redshift (< 0.4) selected from the MCXC cluster catalogue in the Hyper Suprime-Cam Subaru Strategic Program field. We derive the hydrostatic equilibrium mass and study scaling relations using i) the whole sample, ii) only relaxed clusters and iii) only disturbed clusters. When considering the whole sample, the π X -π tot and π gas -π tot relations agree with self-similarity. In terms of morphology, relaxed clusters … Show more
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