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Dark Matter and Cooling Flows

Published online by Cambridge University Press:  03 August 2017

B. J. Carr  and
K. M. Ashman
B. J. Carr
Affiliation:
School of Mathematical Sciences, Queen Mary College, Mile End Road, London E1 4NS
K. M. Ashman
Affiliation:
School of Mathematical Sciences, Queen Mary College, Mile End Road, London E1 4NS

Abstract

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Cosmological arguments suggest that a large fraction of the baryons in the Universe are dark. Although the background dark matter required to make up the critical density would have to consist of some kind of elementary particle, the dark matter in galactic halos could be baryonic. In particular, we argue that it could consist of jupiters made in pregalactic or protogalactic cooling flows. These would be analagous to the cluster cooling flows observed at the present epoch but on a smaller scale.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 429 - 435
Copyright
Copyright © Reidel 1988 

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