Approximate Self-Consistent Models for Tidally Truncated Star Clusters
Astrophysics
2007-05-23 v1
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.
Cite
@article{arxiv.astro-ph/9303010,
title = {Approximate Self-Consistent Models for Tidally Truncated Star Clusters},
author = {D. C. Heggie and N. Ramamani},
journal= {arXiv preprint arXiv:astro-ph/9303010},
year = {2007}
}
Comments
22 pages