Hostname: page-component-586b7cd67f-g8jcs Total loading time: 0 Render date: 2024-11-29T00:02:42.570Z Has data issue: false hasContentIssue false
  • English
  • Français

Formation and Disruption of Globular Star Clusters

Published online by Cambridge University Press:  03 August 2017

S. Michael Fall  and
Qing Zhang
S. Michael Fall
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA
Qing Zhang
Affiliation:
Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, USA

Abstract

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.

In the first part of this article, we review observations of the mass and luminosity functions of young and old star cluster systems. We also review some of the physical processes that may determine the characteristic mass of globular clusters and the form of their mass function. In the second part of this article, we summarize our models for the disruption of clusters and the corresponding evolution of the mass function. Much of our focus here is on understanding why the mass function of globular clusters has no more than a weak dependence on radius within their host galaxies.

Type
Part 4. Star Cluster Formation and Evolution: Theory and Observation
Information
Symposium - International Astronomical Union , Volume 207: Extragalactic Star Clusters , 2002 , pp. 566 - 576
Copyright
Copyright © Astronomical Society of the Pacific 2002 

References

Baumgardt, H. 1998, A&A, 330, 480 Google Scholar
Caputo, F., & Castellani, V. 1984, MNRAS, 207, 185 Google Scholar
Christian, C. A., & Schommer, R. A. 1988, AJ, 95, 704 Google Scholar
Dickey, J. M., & Garwood, R. W. 1989, ApJ, 341, 201 Google Scholar
Dinescu, D. I., Girard, T. M., & van Altena, W. F. 1999, AJ, 117, 1792 CrossRefGoogle Scholar
Elmegreen, B. G., & Efremov, Y. N. 1997, ApJ, 480, 235 Google Scholar
Elson, R. A. W., & Fall, S. M. 1985, PASP, 97, 692 Google Scholar
Fall, S. M., & Rees, M. J. 1977, MNRAS, 181, 37P CrossRefGoogle Scholar
Fall, S. M., & Rees, M. J. 1985, ApJ, 298, 18 Google Scholar
Fall, S. M., & Zhang, Q. 2001, ApJ, in press (astro-ph/0107298) Google Scholar
Frenk, C. S., & White, S. D. M. 1980, MNRAS, 193, 295 Google Scholar
Gnedin, O. Y., & Ostriker, J. P. 1997, ApJ, 474, 223 CrossRefGoogle Scholar
Harris, W. E. 1991, ARA&A, 29, 543 Google Scholar
Harris, W. E. 1996, AJ, 112, 1487 CrossRefGoogle Scholar
Harris, W. E. 1999, http://www.physics.mcmaster.ca/Globular.html Google Scholar
Harris, W. E., & Pudritz, R. E. 1994, ApJ, 429, 177 Google Scholar
Kang, H., Shapiro, P. R., Fall, S. M., & Rees, M. J. 1990, ApJ, 363, 488 CrossRefGoogle Scholar
Solomon, P. M., & Rivolo, A. R. 1989, ApJ, 339, 919 Google Scholar
Spitzer, L. 1987, Dynamical Evolution of Globular Clusters (Princeton: Princeton Univ. Press)Google Scholar
van den Bergh, S., & Lafontaine, A. 1984, AJ, 89, 1822 Google Scholar
Vesperini, E. 1997, MNRAS, 287, 915 Google Scholar
Vesperini, E. 1998, MNRAS, 299, 1019 Google Scholar
Whitmore, B. C., Zhang, Q., Leitherer, C., Fall, S. M., Schweizer, F., & Miller, B. W. 1999, AJ, 118, 1551 CrossRefGoogle Scholar
Zhang, Q., & Fall, S. M. 1999, ApJ, 527, L81 Google Scholar