Baryonic Dark Halos: A Model with MACHOS and Cold Gas Globules
arXiv:astro-ph/9511036
Abstract
The dark matter in the halos of galaxies may well be baryonic, and much of the mass within them could be in the form of clusters of substellar objects within which are embedded cold gas globules. Such halos might play an active role in galaxy formation and evolution.
To be published in the Proceedings of IAU Symposium 171, `New Light on Galaxy Evolution', Eds.: R. Bender and R. Davies. 4 pages, gzip-compressed and uuencoded PS file. Also available at http://www.astro.unibas.ch/~gerhard/papers/iau171_bdm.ps.gz.uu