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Gas in Groups and Clusters of Galaxies
Authors:Sabine Schindler
Institution:1. Institut für Astrophysik, Universit?t Innsbruck, Germany
Abstract:Groups and clusters contain a large fraction of hot gas which emitsX-ray radiation. This gas yields information on the dynamical stateand on the total mass of these systems. X-ray spectra show that heavyelements are present in the gas. As these metals must have beenproduced in the cluster/group galaxies and later transported into thegas, the metallicity is a good tracer for the transport processes. Severalpossible processes, that transport gas from the small potential wellsof the galaxies into the clusters and groups, are discussed.
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