Dark Matter and Cold Fractal Clouds

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dc.creatorTappe, Achim
dc.date2000-06-27
dc.date2000-07-13
dc.date.accessioned2026-07-07T01:54:10Z
dc.date.available2026-07-07T01:54:10Z
dc.descriptionThere is strong evidence for a large fraction of dark matter in the Universe. Some of the evidence and candidates for dark matter are reviewed. Dark matter in spiral galaxies may be in the form of cold dense clouds of molecular hydrogen. This model is presented in more detail and perspectives for detecting the cold H_2 are discussed.
dc.descriptionReview presented at the workshop "Astrophysical Dynamics 1999/2000: Merging Research and Education", Onsala Space Observatory, January 2000, see physics/0006023. 16 pages, 7 figures. Replaced with minor changes in section 2.2.2; one reference added
dc.identifierhttps://arxiv.org/abs/astro-ph/0006393
dc.identifierhttp://arxiv.org/abs/astro-ph/0006393
dc.identifierAstrophysical Dynamics 1999/2000, Alessandro B. Romeo (Ed.), Onsala Space Observatory, 2000, pp. 27-42
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1239
dc.subjectAstrophysics
dc.titleDark Matter and Cold Fractal Clouds
dc.typetext

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