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Globular Clusters and Dark Clusters

Published online by Cambridge University Press:  03 August 2017

Keith M. Ashman*
Affiliation:
Astronomy Unit, School of Maths Sciences, Queen Mary, College, LONDON E1 4NS. U.K.

Abstract

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Fall and Rees have suggested that thermal instability in the collapsing gas of a protogalaxy gives rise to cool clouds embedded in a hot medium. They argue that the temperature of the clouds cannot fall below 104K, since metals and molecular coolants are absent. Clouds with masses exceeding 106M are gravitationally unstable and are identified as the precursors of globular clusters. This model has difficulty in explaining high-metallicity globular clusters, since metals provide cooling down to ∼102K or below, thus considerably reducing the cloud Jeans mass. The same problem arises if H2 cooling occurs.

Type
Appendix 1: Poster Papers
Copyright
Copyright © Reidel 1988 

References

1. Fall, S.M., and Rees, M.J., 1985. Astrophys. J., 298, 18.Google Scholar
2. Carr, B.J., and Lacey, C.G., 1987. Astrophys. J., 316, 23.Google Scholar