Hostname: page-component-76fb5796d-vvkck Total loading time: 0 Render date: 2024-04-26T06:14:47.278Z Has data issue: false hasContentIssue false
  • English
  • Français

Dynamical Evolution of the Mass Function of the Globular Cluster System from Fokker-Planck Calculations: Preliminary Results

Published online by Cambridge University Press:  01 August 2006

Jihye Shin  and
Sungsoo S. Kim
Jihye Shin
Affiliation:
Department of Astronomy and Space Science, Kyung Hee University, Yongin-shi, Kyungki-do 449-701, South Korea email: jhshin@ap1.khu.ac.kr
Sungsoo S. Kim
Affiliation:
Department of Astronomy and Space Science, Kyung Hee University, Yongin-shi, Kyungki-do 449-701, South Korea email: jhshin@ap1.khu.ac.kr
Rights & Permissions [Opens in a new window]

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.

Using anisotropic Fokker-Planck models, we calculate the evolution of mass and luminosity functions of the Galactic globular cluster system. Our models include two-body relaxation, binary heating, tidal shocks, dynamical friction, and stellar evolution. We perform Fokker-Planck simulations for a large number of virtual globular clusters and synthesize these results to study the relation between the initial and present GCMFs.

Keywords

Globular clusterFokker-Planck
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Symposium S235: Galaxy Evolution Across the Hubble Time , August 2006 , pp. 110
Copyright
Copyright © International Astronomical Union 2007

References

Fall, S.M. & Zhang, Q. 2001, ApJ 561, 751.CrossRefGoogle Scholar
Takahashi, K. & Lee, H.M. 2000, ApJ 316, 671.Google Scholar