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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

References

Chevalier, R.A. 1987, Ap.J., 318, 66.Google Scholar
Fabricant, D. and Gorenstein, P. 1983, A;.J., 267, 535.Google Scholar
Gisler, G.R. 1976, Ast. Ap., 51, 137.Google Scholar
Hattori, M., Habe, A. and Ikeuchi, S. 1987, Prog. Theor. Phys., 78, 1099.Google Scholar
Innanen, K.A. 1973, Ap. Space Sci., 22, 393.CrossRefGoogle Scholar
King, R.I. 1972, Ap. J., 174, L123.Google Scholar
Macdonald, J., and Bailey, M.E. 1981 M.N.R.A.S., 197, 995.Google Scholar
Matthews, W.G., and Bregman, J.N. 1978, Ap. J., 224, 308.Google Scholar
Nulsen, P.E.J. 1986 M.N.R.A.S., 221, 377.Google Scholar
Raymond, J.C., Cox, D.P., and Smith, B.W. 1976, Ap. J., 204, 290.Google Scholar
Sarazin, C.L. 1986, Rev. Modern Phys., 58, 1.CrossRefGoogle Scholar
Sarazin, C.L., and White, R.E. III., 1987, Ap. J., 320, 32.Google Scholar
Sargent, W.L.W., Young, P.J., Boksenberg, A., Shortridge, K., Lynds, C.R., and Hartwick, F.D.A. 1978, Ap. J., 221,731.Google Scholar
Stewart, G.C., Canizares, C.R., Fabian, A.C., and Nulsen, P.E.J. 1984, Ap. J., 278, 536.CrossRefGoogle Scholar
Thomas, P.A., Fabian, A.C., and Nulsen, P.E.J. 1987 M.N.R.A.S., 228, 973.CrossRefGoogle Scholar
Tammann, G.A. 1974, in Supernovae: A Survey of Current Research, ed. Comovici, C.B.,Reidel, S., pp 371.Google Scholar
White, R.E. III, and Sarazin, C.L. 1987a, Ap. J., 318, 612.Google Scholar
White, R.E. III, and Sarazin, C.L. 1987b, Ap. J., 318, 621.Google Scholar
White, R.E. III, and Sarazin, C.L. 1987c, Ap. J., 318, 629.Google Scholar