Approximate Self-Consistent Models for Tidally Truncated Star Clusters

D. C. Heggie; N. Ramamani

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Approximate Self-Consistent Models for Tidally Truncated Star Clusters

D. C. Heggie·N. Ramamani

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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.

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D. C. Heggie, N. Ramamani. 1993-03-19. Approximate Self-Consistent Models for Tidally Truncated Star Clusters. https://arxiv.org/abs/astro-ph/9303010

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