Hostname: page-component-7bb8b95d7b-nptnm Total loading time: 0 Render date: 2024-09-18T15:18:55.730Z Has data issue: false hasContentIssue false

The Origin of Globular Clusters

Published online by Cambridge University Press:  19 July 2016

S. Michael Fall
Affiliation:
Space Telescope Science Institute and Johns Hopkins University
Martin J. Rees
Affiliation:
Institute of Astronomy, Cambridge

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The purpose of this article is to review some recent attempts to understand the origin of globular clusters. To put this in perspective, it may help to recall the analogous problem of the origin of galaxies. This splits into two parts. First, given a proto-galaxy with a specified mass and radius, how does it collapse, form stars and settle into a state of dynamical equilibrium? Richard Larson explored these topics in an important series of numerical simulations in the 1970s. Progress in this area brings into sharper focus a second set of questions that really has precedence over the first. Why did proto-galaxies have properties like the initial conditions in the collapse calculations and what distinguishes galaxies from structures on much larger and much smaller scales? Similar questions face us when we consider the origin of globular clusters. First, how did stars form in a proto-cluster, what was the efficiency, the initial mass function and so forth? It is appropriate that Larson has discussed these topics in the preceding article but here we are mainly concerned with the second kind of question: What is special about objects with masses of order 105-106 M and dimensions of a few tens of parsecs?

Type
Chapter IV. Review Papers on Evolution of Globular Clusters
Copyright
Copyright © Kluwer 1988 

References

REFERENCES

Binney, J. 1977 Astrophys. J. 215, 483.Google Scholar
Blumenthal, G. R., Faber, S. M., Primack, J. R. and Rees, M. J. 1984 Nature 311, 517.Google Scholar
Caputo, F. and Castellani, V. 1984 Monthly Notices Roy. Astron. Soc. 207, 185.Google Scholar
Elson, R. A. W. and Fall, S. M. 1985a Publ. Astron. Soc. Pacific 97, 692.Google Scholar
Elson, R. A. W. and Fall, S. M. 1985b Astrophys. J. 299, 211.Google Scholar
Fabian, A. C., Nulsen, P. E. J. and Canizares, C. R. 1984 Nature 310, 733.Google Scholar
Fall, S. M. 1986 in preparation.Google Scholar
Fall, S. M. and Rees, M. J. 1977 Monthly Notices Roy. Astron. Soc. 181, 37p.CrossRefGoogle Scholar
Fall, S. M. and Rees, M. J. 1985 Astrophys. J. 298, 18.Google Scholar
Forte, J. C., Strom, S. E. and Strom, K. M. 1981 Astrophys. J. Letters 245, L9.Google Scholar
Freeman, K. C., Illingworth, G. and Oemler, A. 1983 Astrophys. J. 272, 488.CrossRefGoogle Scholar
Gunn, J. E. 1980 in Globular Clusters Hanes, D. and Madore, B., eds., Cambridge University Press, Cambridge, p. 301.Google Scholar
Harris, W. E. 1986 Astrophys. J., 91, 822.Google Scholar
Larson, R. B. 1986 in Nearly Normal Galaxies : From the Planck Time to the Present Faber, S. M., ed., Springer-Verlag, New York, in press.Google Scholar
McCrea, W. H. 1982 in Progress in Cosmology Wolfendale, A. W., ed., Reidel, Dordrecht, p. 239.Google Scholar
Mould, J. 1986 in Stellar Populations Norman, C. A., Renzini, A. and Tosi, M., Cambridge University Press, Cambridge, in press.Google Scholar
Mould, J. R., Oke, J. B. and Nemec, J. M. 1986 preprint.Google Scholar
Oort, J. H. 1965 in Stars and Stellar Systems. Vol. 5. Galactic Structure Blaau, A. and Schmidt, M., eds, University of Chicago Press, Chicago, p. 455.Google Scholar
Peebles, P. J. E. 1984 Astrophys. J. 277, 470.Google Scholar
Peebles, P. J. E. and Dicke, R. H. 1968 Astrophys. J. 154, 891.Google Scholar
Rees, M. J. and Ostriker, J. P. 1977 Monthly Notices Roy. Astron. Soc. 179, 541.Google Scholar
Rogers, A. W. and Paltoglou, G. 1984 Astrophys. J. Letters 283, L5.Google Scholar
Searle, L. 1977 in The Evolution of Galaxies and Stellar Populations Tinsley, B. M. and Larson, R. B., eds, Yale University Observatory, New Haven, p. 219.Google Scholar
Searle, L. and Zinn, R. 1978 Astrophys. J., 225, 357.Google Scholar
Silk, J. 1977 Astrophys. J., 211, 638.Google Scholar
Stecher, T. P. and Williams, D. A. 1967 Astrophys. J. Letters 149, L29.Google Scholar
Stewart, G. C., Canizares, C. R., Fabian, A. C. and Nulsen, P. E. J. 1984 Astrophys. J. 278, 536.CrossRefGoogle Scholar
White, S. D. M. and Rees, M. J. 1978 Monthly Notices Roy. Astron. Soc. 183, 341.CrossRefGoogle Scholar
Zinn, R. 1985 Astrophys. J. 293, 424.Google Scholar