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Issue A&A
Volume 454, Number 3, August II 2006
Page(s) L131 - L134
Section Letters
DOI http://dx.doi.org/10.1051/0004-6361:20065404



A&A 454, L131-L134 (2006)
DOI: 10.1051/0004-6361:20065404

Letter

The impact of magnetic field on the cluster M - T relation

S. Colafrancesco and F. Giordano

INAF - Osservatorio Astronomico di Roma, via Frascati 33, 00040 Monteporzio, Italy
    e-mail: cola@mporzio.astro.it

(Received 10 April 2006 / Accepted 8 June 2006 )

Abstract
We discuss the impact of magnetic field on the mass-temperature relation for groups and clusters of galaxies based on the derivation of the general Magnetic Virial Theorem. The presence of a magnetic field B yields a decrease of the virial temperature T for a fixed mass M: such a decrease in T is stronger for low-mass systems than for high-mass systems. We outline several implications of the presence of B-field and of its mass scaling for the structure and evolution of groups and clusters.


Key words: cosmology: theory -- galaxies: clusters: general -- magnetic field



© ESO 2006


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