Dissolution of globular clusters

Baumgardt, H (2009). Dissolution of globular clusters. In: Tom Richtler, Søren Larsen and Bruno Leibundgut, Globular Clusters: Guides to Galaxies. Proceedings of the Joint ESO-FONDAP Workshop on Globular Clusters. FONDAP-ESO Conference. Globular Clusters: Guides to Galaxies, Concepción, Chile, (387-394). 6-10 March 2006. doi:10.1007/978-3-540-76961-3_89


Author Baumgardt, H
Title of paper Dissolution of globular clusters
Conference name FONDAP-ESO Conference. Globular Clusters: Guides to Galaxies
Conference location Concepción, Chile
Conference dates 6-10 March 2006
Proceedings title Globular Clusters: Guides to Galaxies. Proceedings of the Joint ESO-FONDAP Workshop on Globular Clusters
Journal name ESO Astrophysics Symposia
Place of Publication Heidelberg, Germany
Publisher Springer
Publication Year 2009
Sub-type Fully published paper
DOI 10.1007/978-3-540-76961-3_89
ISBN 9783540769606
3540769609
9783540769613
3540769617
9783642095658
3642095658
ISSN 1431-2433
Editor Tom Richtler
Søren Larsen
Bruno Leibundgut
Volume 47
Start page 387
End page 394
Total pages 8
Language eng
Formatted Abstract/Summary
Globular clusters are among the oldest objects in galaxies, and understanding the details of their formation and evolution can bring valuable insight into the early history of galaxies. Until the late 1970s, globular clusters were thought of to be relatively static stellar systems, a view which was supported by the fact that most observed density profiles of globular clusters can be fitted with equilibrium models like e.g. King profiles. This view has changed significantly over the last twenty years. On the observational side, the evidence for differences in the stellar mass-functions of globular clusters, which are believed to be at least partly the result of their dynamical evolution, and the discovery of extratidal stars surrounding globular clusters are strong indications for the ongoing dynamical evolution and dissolution of globular clusters.

On the theoretical side, N-body simulations of star cluster evolution have become increasingly sophisticated, due to both progresses in simulation techniques and the development of the GRAPE series of special purpose computers, which allows to simulate the evolution of star clusters with increasingly larger particle numbers.

This review summarises the current knowledge about the dissolution of star clusters and discusses the implications of star cluster dissolution for the evolution of the mass function of star cluster systems in galaxies.
Keyword Initial mass function
Special-purpose computer
Monte-Carlo simulations
Star-clusters
Dynamical evolution
Stellar evolution
Tidal fields
Systems
Disruption
Galaxies
Q-Index Code E1
Q-Index Status Provisional Code
Institutional Status Non-UQ

Document type: Conference Paper
Collections: School of Mathematics and Physics
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