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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1787
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dc.contributor.authorBhatnagar, K. B-
dc.contributor.authorHallan, P. P-
dc.date.accessioned2007-09-14T07:12:20Z-
dc.date.available2007-09-14T07:12:20Z-
dc.date.issued1995-
dc.identifier.citationBASI, Vol. 23, No. 2, pp. 177-194en
dc.identifier.urihttp://hdl.handle.net/2248/1787-
dc.description.abstractThe non-linear stability of an ellipsoidal cluster of stars sharing galactic rotation has been studied. It is seen that the cluster is stable for all densities in the range of linear stability except for those satisfying certain equations where Arnold's theorem is not applicable.en
dc.format.extent652410 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995BASI...23..177Ben
dc.subjectArnold's theoremen
dc.subjectstabilityen
dc.subjectcluster of starsen
dc.titleNon-linear stability of a cluster of stars sharing galactic rotationen
dc.typeArticleen
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