Approximate Self-Consistent Models for Tidally Truncated Star Clusters

Details Approximate Self-Consistent Models for Tidally Truncated Star Clusters Approximate Self-Consistent Models for Tidally Truncated Star Clusters

1993-03-19

arxiv.org/abs/astro-ph/9303010v1

Astronomy and Astrophysics

Astrophysics

22 pages

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Approximate Self-Consistent Models for Tidally Truncated Star Clusters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Approximate Self-Consistent Models for Tidally Truncated Star Clusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Approximate Self-Consistent Models for Tidally Truncated Star Clusters will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-221006