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The Dynamics of Globular Cluster Systems
Published online by Cambridge University Press: 19 July 2016
Abstract
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
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- Copyright
- Copyright © Kluwer 1988