A note on Temperature Profiles of rich Clusters of Galaxies

Details A note on Temperature Profiles of rich Clusters of Galaxies A note on Temperature Profiles of rich Clusters of Galaxies

2004-07-19

arxiv.org/abs/astro-ph/0407392v1

Astronomy and Astrophysics

Astrophysics

3 pages, 2 figures included. Proceedings of IAU Colloquium n.195 - Outskirts of Galaxy Clusters: intense life in the suburbs

Scientific paper

10.1017/S1743921304000298

We derive here the mean temperature profile for a sample of hot, medium distant clusters recently observed with XMM-Newton, whose profiles are available from the literature, and compare it with the mean temperature profile found from BeppoSAX data. The XMM-Newton and BeppoSAX profiles are in good agreement between 0.05 and 0.25 r_180. From 0.25 to about 0.5 r_180 both profiles decline, however the BeppoSAX profile does so much more rapidly than the XMM-Newton profile.

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