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A note on Temperature Profiles of rich Clusters of Galaxies

Sabrina De Grandi·Silvano Molendi
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Abstract

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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Sabrina De Grandi, Silvano Molendi. 2004-07-19. A note on Temperature Profiles of rich Clusters of Galaxies. https://doi.org/10.1017/s1743921304000298

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