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Baryonic Dark Halos: a model with MACHOS and cold gas globules

Published online by Cambridge University Press:  25 May 2016

Ortwin Gerhard  and
Joseph Silk
Ortwin Gerhard
Affiliation:
Astronomisches Institut, Univ. Basel, Switzerland
Joseph Silk
Affiliation:
Dpt. of Astronomy, Univ. of California, Berkeley, U.S.A.

Abstract

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The dark matter in the halos of galaxies may well be baryonic, and much of the mass within them could be in the form of clusters of substellar objects within which are embedded cold gas globules. Such halos might play an active role in galaxy formation and evolution.

Type
Dark Matter Halos around Galaxies
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 167 - 170
Copyright
Copyright © Kluwer 1996 

References

Alcock, C. A., et al., 1993, Nature 365, 621 CrossRefGoogle Scholar
Alcock, C. A., et al., 1995, ApJ, in press Google Scholar
Aubourg, E., et al., 1993, Nature 365, 623 Google Scholar
Bosma, A., 1981, AJ 86, 1825 Google Scholar
Gerhard, O.E., Silk, J., 1995, ApJ, submitted Google Scholar
Kolb, E.W., Turner, M.S., 1990, The Early Universe (Addison Wesley, New York).Google Scholar
Moore, B., Silk, J., 1995, ApJ 442, L5 Google Scholar
Neufeld, D.A., Lepp, S., Melnick, G.J., 1995, preprint.Google Scholar
Rees, M.J., 1976, MNRAS 176, 483 Google Scholar