Baryonic dark matter

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dc.creatorDe Paolis, F.
dc.creatorIngrosso, G.
dc.creatorJetzer, Ph.
dc.creatorRoncadelli, M.
dc.date1996-10-04
dc.date.accessioned2026-07-07T02:22:01Z
dc.date.available2026-07-07T02:22:01Z
dc.descriptionReasons supporting the idea that most of the dark matter in galaxies and clusters of galaxies is baryonic is discussed. Moreover it is argued that most of the dark matter in galactic halo should be in the form of MACHOs and cold molecular clouds.
dc.descriptionTo appear in "Dark and visible matter in galaxies and cosmological implications" eds. M. Persic and P.Salucci A.S.P. conference series
dc.identifierhttps://arxiv.org/abs/astro-ph/9610031
dc.identifierhttp://arxiv.org/abs/astro-ph/9610031
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10719
dc.subjectAstrophysics
dc.titleBaryonic dark matter
dc.typetext

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