Non-linear stability of a cluster of stars sharing galactic rotation

dc.contributor.author	Bhatnagar, K. B
dc.contributor.author	Hallan, P. P
dc.date.accessioned	2007-09-14T07:12:20Z
dc.date.available	2007-09-14T07:12:20Z
dc.date.issued	1995
dc.identifier.citation	BASI, Vol. 23, No. 2, pp. 177-194	en
dc.identifier.uri	http://hdl.handle.net/2248/1787
dc.description.abstract	The 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.extent	652410 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1995BASI...23..177B	en
dc.subject	Arnold's theorem	en
dc.subject	stability	en
dc.subject	cluster of stars	en
dc.title	Non-linear stability of a cluster of stars sharing galactic rotation	en
dc.type	Article	en