Origins, levels and effects of non-gravitational energy inputs into the ICM pervading groups and clusters of galaxies. The role of the SZ effect as a probe of these processes.

The thermal state of the ICM probed with the SZ effect / Cavaliere, A.; Lapi, A.; Menci, N.. - 268:(2002), pp. 240-247.

The thermal state of the ICM probed with the SZ effect

Cavaliere, A.;Lapi, A.;
2002-01-01

Abstract

Origins, levels and effects of non-gravitational energy inputs into the ICM pervading groups and clusters of galaxies. The role of the SZ effect as a probe of these processes.
2002
Tracing Cosmic Evolution with Galaxy Clusters
268
240
247
1-58381-108-7
http://www.aspbooks.org/a/volumes/article_details/?paper_id=24995
Astronomical Society of the Pacific Conference Ser
Cavaliere, A.; Lapi, A.; Menci, N.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/15488
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