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Gas in Groups and Clusters of Galaxies

Name: Gas in Groups and Clusters of Galaxies
Creator: Sabine Schindler
Keywords: Astrophysics (astro-ph), 0103 physical sciences, FOS: Physical sciences, Astrophysics, 01 natural sciences

descriptionPublicationkeyboard_double_arrow_right Part of book or chapter of book , Article , Preprint , Other literature type 01 Jan 2004Embargo end date: 01 Jan 2002 English Publisher:Springer NetherlandsJournal:Astrophysics and Space Science, volume 289, pages 419-428 (issn: 0004-640X, eissn: 1572-946X,

Authors: Sabine Schindler;

doi: 10.1007/978-94-007-0979-9_35 , 10.1023/b:astr.0000014973.75505.0f , 10.48550/arxiv.astro-ph/0212104

arXiv: http://arxiv.org/abs/astro-ph/0212104

Gas in Groups and Clusters of Galaxies

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Abstract

Groups and clusters contain a large fraction of hot gas which emits X-ray radiation. This gas yields information on the dynamical state and on the total mass of these systems. X-ray spectra show that heavy elements are present in the gas. As these metals must have been produced in the cluster/group galaxies and later transported into the gas, the metallicity is a good tracer for the transport processes. Several possible processes, that transport gas from the small potential wells of the galaxies into the clusters and groups, are discussed.

Invited review given at the JENAM 2002 in Porto, Workshop ISM, eds. M.A. de Avillez & D. Breitschwerdt, Kluwer, 10 pages, 7 figures

Related Organizations

University of Innsbruck
Austria

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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