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Gas in Galaxy Clusters

Published online by Cambridge University Press:  14 August 2015

Joseph Silk
Joseph Silk*
Affiliation:
Department of Astronomy, University of California Berkeley, California 94720

Extract

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Gaseous matter almost certainly cannot account for a significant amount of the binding mass in the cores of rich clusters. Implications of the variety of upper limits are well known (Tarter and Silk 1974), and will not be described here. However intracluster gas provides important clues to the evolution of galaxy clusters, and the present review is devoted to elucidating its role.

Type
II. Clusters of Galaxies
Information
Symposium - International Astronomical Union , Volume 79: The Large Scale Structure of the Universe , 1978 , pp. 179 - 188
Copyright
Copyright © Reidel 1978 

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