Hostname: page-component-7479d7b7d-wxhwt Total loading time: 0 Render date: 2024-07-13T13:29:26.893Z Has data issue: false hasContentIssue false
  • English
  • Français

Cooling Flows and the Formation of Dark matter

Published online by Cambridge University Press:  04 August 2017

A. C. Fabian ,
K. A. Arnaud  and
P. A. Thomas
A. C. Fabian
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, United Kingdom
K. A. Arnaud
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, United Kingdom
P. A. Thomas
Affiliation:
Institute of Astronomy, Madingley Road, Cambridge CB3 OHA, United Kingdom

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The distribution of matter condensing out of cooling flows in clusters of galaxies and individual elliptical galaxies has been studied using X-ray data and is found to resemble the expected mass profiles of the underlying galaxies. Most of the cooled gas must create objects of high mass-to-light ratio, although some more normal stars are produced. Cooling flows provide an observable mechanism for the continual formation of dark matter around galaxies. Since the conditions at galaxy formation are similar to those in cooling flows if the gas reaches the virial temperature, we suggest that they are local models of galaxy formation.

Type
Review Paper
Information
Symposium - International Astronomical Union , Volume 117: Dark Matter in the Universe , 1987 , pp. 201 - 213
Copyright
Copyright © Reidel 1987 

References

Arnaud, K.A. & Gilmore, G.: 1985, preprint.Google Scholar
Arnaud, K.A., Fabian, A.C., Eales, S.A., Jones, C. & Forman, W.: 1984, M.N.R.A.S. 211, 981.CrossRefGoogle Scholar
Butcher, A.R. & Oemler, A.: 1984, Nature, 310, 31.Google Scholar
Canizares, C.R.: 1981, X-ray Astronomy with the Einstein Satellite, ed. Giacconi, R., Reidel, 215.Google Scholar
Canizares, C.R., Stewart, G.C. & Fabian, A.C.: 1983, Ap. J., 272, 449.Google Scholar
Canizares, C.R.: 1986, this volume.Google Scholar
Cowie, L.L., Fabian, A.C. & Nulsen, P.E.J.: 1980, M.N.R.A.S., 191, 399.CrossRefGoogle Scholar
Cowie, L.L., Hu, E.M., Jenkins, E.B. & York, D.G.: 1983, Ap. J., 272, 29.Google Scholar
Crane, P.C., van der Hulst, J.M. & Haschick, A.D.: 1982, IAU Symposium 97, eds. Heeschen, D.S. & Wade, C.M., 307.Google Scholar
Fabian, A.C., Hu, E.M., Cowie, L.L., Grindlay, J.: 1981, Ap. J., 248, 47.CrossRefGoogle Scholar
Fabian, A.C., Nulsen, P.E.J. & Canizares, C.R.: 1982, M.N.R.A.S., 201, 933.CrossRefGoogle Scholar
Fabian, A.C., Nulsen, P.E.J. & Arnaud, K.A.: 1984, M.N.R.A.S., 208, 179.Google Scholar
Fabian, A.C., Nulsen, P.E.J. & Canizares, C.R.: 1984, Nature, 310, 733.Google Scholar
Fabian, A.C., Arnaud, K.A., Nulsen, P.E.J., Watson, M.G., Stewart, G.C., McHardy, I., Smith, A., Cooke, B., Elvis, M. & Mushotzky, R.F.: 1985, M.N.R.A.S., in press.Google Scholar
Fabian, A.C., Arnaud, K.A., Nulsen, P.E.J. & Mushotzky, R.F.: 1985b, Ap. J., submitted.Google Scholar
Fabricant, D. & Gorenstein, P.: 1983, Ap. J., 267, 535.CrossRefGoogle Scholar
Forman, W., Jones, C. & Tucker, W.: 1985, Ap. J., 293, 102.Google Scholar
Gear, W.K., Gee, G., Robson, E.I. & Nolt, I.G.: M.N.R.A.S., in press.Google Scholar
Jones, C. & Forman, W.: 1984, Ap. J., 276, 38.Google Scholar
Kent, S.M. & Sargent, W.L.W.: 1979, Ap. J., 230, 667.Google Scholar
Lilly, S. & Longair, M.S.: 1984, M.N.R.A.S., 211, 833.Google Scholar
Low, C. & Lynden-Bell, D.: 1976, M.N.R.A.S., 176, 367.CrossRefGoogle Scholar
Lynds, R.: 1970, Ap. J., 159, L151.Google Scholar
McGlynn, T.A. & Fabian, A.C.: 1984, M.N.R.A.S., 208, 709.Google Scholar
Mushotzky, R.F., Holt, S.S., Smith, B.W., Boldt, E.A. & Serlemitsos, P.J.: 1981, Ap. J., 244, L47.Google Scholar
Nulsen, P.E.J., Stewart, G.C. & Fabian, A.C.: 1984, M.N.R.A.S., 208, 185.Google Scholar
Raymond, J. & Smith, B.W.: 1977, Ap. J. Supp. Google Scholar
Rees, M.J. & Ostriker, J.: 1977, M.N.R.A.S., 179, 541.Google Scholar
Rubin, V.C., Ford, W.K., Peterson, C.J. & Oort, J.H.: 1977, Ap. J., 211, 693.Google Scholar
Sarazin, C.L. & O'Connell, R.W.: 1983, Ap. J., 268, 552.Google Scholar
Sarazin, C.L.: 1985, Rev. Mod. Phys., in press.Google Scholar
Sarazin, C.L.: 1986, this volume.Google Scholar
Silk, J.: 1977, Ap. J., 211, 638.Google Scholar
Spinrad, H. & Djorgovski, G.: 1984a, Ap. J., 280, L9.Google Scholar
Spinrad, H. & Djorgovski, G.: 1984b, Ap. J., 285, L49.CrossRefGoogle Scholar
Stewart, G.C., Canizares, C.R., Fabian, A.C. & Nulsen, P.E.J.: 1984a, Ap. J., 278, 536.Google Scholar
Stewart, G.C., Fabian, A.C., Jones, C. & Forman, W.: 1984b, Ap. J., 285, 1.Google Scholar
Thomas, , et al.: 1985, preprint.Google Scholar
White, R.E. & Chevalier, R.A.: 1983, Ap. J., 275, 1983.Google Scholar