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Baryonic Dark Halos: A Model with Machos and Cold Gas Globules

  • Ortwin Gerhard
  • Joseph Silk
Conference paper
Part of the International Astronomical Union / Union Astronomique Internationale book series (IAUS, volume 171)

Abstract

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.

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References

  1. Alcock, C. A., et al., 1993, Nature 365, 621ADSCrossRefGoogle Scholar
  2. Alcock, C. A., et al., 1995, ApJ, in pressGoogle Scholar
  3. Aubourg, E., et al., 1993, Nature 365, 623ADSCrossRefGoogle Scholar
  4. Bosma, A., 1981, AJ 86, 1825ADSCrossRefGoogle Scholar
  5. Gerhard, O.E., Silk, J., 1995, ApJ, submittedGoogle Scholar
  6. Kolb, E.W., Turner, M.S., 1990, The Early Universe (Addison Wesley, New York).zbMATHGoogle Scholar
  7. Moore, B., Silk, J., 1995, ApJ 442, L5ADSCrossRefGoogle Scholar
  8. Neufeld D.A., Lepp S., Melnick G.J., 1995, preprint.Google Scholar
  9. Rees, M.J., 1976, MNRAS 176, 483ADSGoogle Scholar

Copyright information

© Springer Science+Business Media Dordrecht 1996

Authors and Affiliations

  • Ortwin Gerhard
    • 1
  • Joseph Silk
    • 2
  1. 1.Astronomisches InstitutUniv. BaselSwitzerland
  2. 2.Dpt. of AstronomyUniv. of CaliforniaBerkeleyUSA

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