Approximate Self-Consistent Models for Tidally Truncated Star Clusters

Simple item page
dc.creatorHeggie, D. C.
dc.creatorRamamani, N.
dc.date1993-03-19
dc.date.accessioned2026-07-07T02:18:44Z
dc.date.available2026-07-07T02:18:44Z
dc.descriptionThis 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.
dc.description22 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/9303010
dc.identifierhttp://arxiv.org/abs/astro-ph/9303010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9606
dc.subjectAstrophysics
dc.titleApproximate Self-Consistent Models for Tidally Truncated Star Clusters
dc.typetext

Files

Collections

arXiv