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The Evolution of Cooling Flow and the Mass Deposition Process

Published online by Cambridge University Press:  12 April 2016

Makoto Hattori  and
Asao Habe
Makoto Hattori
Affiliation:
Department of Physics, Hokkaido University, Sapporo 060, Japan
Asao Habe
Affiliation:
Department of Physics, Hokkaido University, Sapporo 060, Japan

Abstract

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We perform the numerical hydrodynamical calculation of cluster cooling flow including the mass deposition process and examine evolution of cooling flow. We take two mass deposition models. In one model, mass deposition occurs in large extent. In other model, mass deposition occurs only in central region. In any model, diagnostics of X-ray surface brightness do not agree with observation in any evolutional phases.

Type
6. Clusters of Galaxies, Cooling Flows
Information
International Astronomical Union Colloquium , Volume 115: High Resolution X-ray Spectroscopy of Cosmic Plasmas , 1990 , pp. 255 - 258
Copyright
Copyright © Cambridge University Press 1990

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