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

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.272..317h&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 272, Issue 2, pp. 317-322.

Astronomy and Astrophysics

Astronomy

37

Gravitation-Methods, Numerical-Celestial Mechanics, Stellar Dynamics-Globular Clusters, General-Open Clusters And Associations, General-Galaxies, Star Clusters.

Scientific paper

This paper generalizes 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.

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