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Globular Clusters and Dark Clusters
Published online by Cambridge University Press: 03 August 2017
Abstract
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.
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- Appendix 1: Poster Papers
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- Copyright © Reidel 1988