Chandra Sample of Galaxy Clusters at z=0.4-0.55: Evolution in the Mass-Temperature Relation

Details Chandra Sample of Galaxy Clusters at z=0.4-0.55: Evolution in the Mass-Temperature Relation Chandra Sample of Galaxy Clusters at z=0.4-0.55: Evolution in the Mass-Temperature Relation

2005-11-01

arxiv.org/abs/astro-ph/0511044v1

Astrophys.J.641:752-755,2006

Astronomy and Astrophysics

Astrophysics

Submitted to ApJ Letters. 4 emulateapj pages

Scientific paper

10.1086/500553

We present spatially-resolved analysis of the temperature and gas density profiles in 6 relaxed galaxy clusters at z = 0.4-0.54 using long-exposure Chandra observations. We derived the total cluster masses within the radius r_500 assuming hydrostatic equilibrium but without assuming isothermality of the intracluster gas. Together with a similar study based on the XMM-Newton observations (Kotov & Vikhlinin), we obtained the mass and temperature measurements for 13 galaxy clusters at 0.4

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