Baryonic dark matter

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De Paolis, F. ; Ingrosso, G. ; Jetzer, Ph. ; Roncadelli, M. (1996)
  • Subject: Astrophysics
    arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics

Reasons supporting the idea that most of the dark matter in galaxies and clusters of galaxies is baryonic are discussed. Moreover, it is argued that most of the dark matter in galactic halos should be in the form of MACHOs and cold molecular clouds.
  • References (15)
    15 references, page 1 of 2

    Adams, F. C. & Laughlin, G. 1996, astro-ph/9602006 Alcock, C. et al. 1993, Nature, 365, 621

    Alcock, C. et al. 1996, astro-ph 9606165

    Ashman, K. M. 1992, PASP, 104, 1109

    Aubourg, E. et al. 1993, Nature, 365, 623

    Bahcall, J., Flynn, C., Gould, A & Kirhakos, S. 1994, ApJ, 435, L51 Bahcall, N. A., Lubin, L.M. & Dorman, V. 1995, ApJ, 447, L81 Blumenthal, G. R., Faber, S. M., Primack, J. R. & Rees, M. J. 1984, Nature, 311, 517

    Burkert, A. 1995, ApJ 447, L25

    Carignan, C. & Beaulieu, S. 1989, ApJ 347, 760 Carignan, C. & Freeman, K. C. 1988, ApJ 332, L33 Casertano, S. & Van Gorkom, J. H. 1991, ApJ 101, 1231 Copi, C. J., Schramm, D. N. & Turner, M. S. 1995, Science, 267, 192 De Paolis, F., Ingrosso, G. & Jetzer, Ph. 1996, ApJ October 10, 1996 issue (in press)

    De Paolis, F., Ingrosso, G., Jetzer, Ph. & Roncadelli, M. 1995a, Phys. Rev. Lett., 74, 14

    De Paolis, F., Ingrosso, G., Jetzer, Ph. & Roncadelli, M. 1995b, Astron. & Astrophys. 295, 567

    De Paolis, F., Ingrosso, G., Jetzer, Ph. & Roncadelli, M. 1995c, Comm. Astrophys., 18, 87

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