2000/06/30 by Achim Tappe
Physics and Astronomy · #astro-ph
published as Astrophysical Dynamics 1999/2000, Alessandro B. Romeo (Ed.), Onsala Space Observatory, 2000, pp. 27-42 · Review 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
arxiv created 2000/07/13 · arxiv updated 2009/12/01
There 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 H2 are discussed.