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A note on temperature profiles of rich clusters of galaxies

Published online by Cambridge University Press:  06 October 2004

Sabrina De Grandi  and
Silvano Molendi
Sabrina De Grandi
Affiliation:
INAF OAB, via E. Bianchi 46, 23807 Merate (LC), Italy email: degrandi@mi.astro.it
Silvano Molendi
Affiliation:
IASF, Sez. di Milano, Via Bassini 15, I-20133 Milano, Italy email: silvano@mi.iasf.cnr.it
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Abstract

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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.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Information

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2004 , Issue IAUC195 , March 2004 , pp. 134 - 136
Copyright
© 2004 International Astronomical Union