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The Dynamics of Globular Cluster Systems

Published online by Cambridge University Press:  19 July 2016

Natarajan Ramamani
Natarajan Ramamani*
Affiliation:
University of Edinburgh

Abstract

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This paper describes a project whose aim is to study the dynamics of a globular cluster system using an N-body code modified to include the gravitational field of an isothermal galaxy model. The galaxy and the globular cluster system have the same radii, are spherically symmetric and non-rotating. The evolution is to be followed up to a Hubble time.

Type
Chapter IX. Poster Papers on Cluster Systems in Distant Galaxies. Deep Photometry and CM Diagrams
Information
Symposium - International Astronomical Union , Volume 126: The Harlow-Shapley Symposium on Globular Cluster Systems in Galaxies , 1988 , pp. 641 - 642
Copyright
Copyright © Kluwer 1988 

References

REFERENCES

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Ostriker, J. P. and Caldwell, J. A. R. 1980 in IAU Symposium No. 84. Large-Scale Characteristics of the Galaxy, Burton, W. B., ed., Reidel, Dordrecht, P. 441.Google Scholar