Approximate Self-Consistent Models for Tidally Truncated Star Clusters

Preprint

19 March 1993

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9303010

Abstract

This paper generalises King's models for tidally truncated star clusters by including approximately the non-spherical symmetry of the tidal field and the resulting non-spherical distortion of the cluster.

Keywords

MODELS FOR TIDALLY
TIDALLY TRUNCATED
CONSISTENT MODELS
TRUNCATED STAR
STAR CLUSTERS
APPROXIMATE
DISTORTION

All Related Versions

Version 1, 1993-03-19, ArXiv

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