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.
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© 1996 Springer Science+Business Media Dordrecht
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Gerhard, O., Silk, J. (1996). Baryonic Dark Halos: A Model with Machos and Cold Gas Globules. In: Bender, R., Davies, R.L. (eds) New Light on Galaxy Evolution. International Astronomical Union / Union Astronomique Internationale, vol 171. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0229-9_23
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DOI: https://doi.org/10.1007/978-94-009-0229-9_23
Publisher Name: Springer, Dordrecht
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