Baryonic Dark Matter

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dc.creatorDe Paolis, F.
dc.creatorJetzer, Ph.
dc.creatorIngrosso, G.
dc.creatorRoncadelli, M.
dc.date1997-08-24
dc.date.accessioned2026-07-07T02:24:04Z
dc.date.available2026-07-07T02:24:04Z
dc.descriptionReasons 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.
dc.description3 pages, to appear in Proceedings of the 8th Marcel Grosmann Meeting on relativistic Astrophysics, Jerusalem, 22-27 June 1997
dc.identifierhttps://arxiv.org/abs/astro-ph/9708222
dc.identifierhttp://arxiv.org/abs/astro-ph/9708222
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11490
dc.subjectAstrophysics
dc.titleBaryonic Dark Matter
dc.typetext

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