Approximate Self-Consistent Models for Tidally Truncated Star Clusters
天体物理学
2007-05-23 v1
摘要
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.
引用
@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}
}
备注
22 pages