期刊
ASTRONOMY & ASTROPHYSICS
卷 454, 期 3, 页码 L131-L134出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20065404
关键词
cosmology : theory; galaxies : clusters : general; magnetic field
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.
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