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Clusters of Galaxies and the Hot Intracluster Medium

Published online by Cambridge University Press:  12 April 2016

C. Jones ,
W. Forman  and
L. David
C. Jones
Affiliation:
Harvard/Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA
W. Forman
Affiliation:
Harvard/Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA
L. David
Affiliation:
Harvard/Smithsonian Center for Astrophysics, 60 Garden St., Cambridge, MA

Abstract

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The luminous material in clusters of galaxies falls primarily into two forms — the visible galaxies and the X-ray emitting intracluster medium. The hot intracluster medium is the major observed baryonic component of clusters with a mass equal to or greater than that of the stellar matter. In this paper we discuss changes in the efficiency of galaxy formation for different clusters and the origin of the intracluster medium.

Type
6. Clusters of Galaxies, Cooling Flows
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 249 - 254
Copyright
Copyright © Cambridge University Press 1990

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