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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1788
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dc.contributor.authorHaque, M. N-
dc.contributor.authorIshwar, B-
dc.date.accessioned2007-09-14T07:35:15Z-
dc.date.available2007-09-14T07:35:15Z-
dc.date.issued1995-
dc.identifier.citationBASI, Vol. 23, No. 2, pp. 195-210en
dc.identifier.urihttp://hdl.handle.net/2248/1788-
dc.description.abstractWe have examined the non-linear stability of triangular equilibrium point in the perturbed photogravitaional restricted three body problem. We conclude that the equilibrium point is stable in the range of linear stability except for three mass ratio.en
dc.format.extent628154 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1995BASI...23..195Hen
dc.subjectstabilityen
dc.subjectphotogravitationalen
dc.subjectRTBPen
dc.titleNon-linear stability in the perturbed photogravitational restricted three body problemen
dc.typeArticleen
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