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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2193
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dc.contributor.authorSahoo, S. K-
dc.contributor.authorIshwar, B-
dc.date.accessioned2008-04-02T11:59:32Z-
dc.date.available2008-04-02T11:59:32Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 3, pp. 579 - 586en
dc.identifier.urihttp://hdl.handle.net/2248/2193-
dc.description.abstractWe have examined stability of collinear equilibrium points in the generalised photogravitational elliptic restricted three body problem. The problem is generalised in the sense that the smaller primary is considered as an oblate spheroid and the bigger primary is taken as a source of radiation. We have found the characteristic equation of the problem. We conclude that collinear equilibrium points are unstableen
dc.format.extent403217 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..579Sen
dc.subjectStabilityen
dc.subjectCollinear pointsen
dc.subjectGeneralised photogravitationalen
dc.subjectERTBPen
dc.titleStability of collinear equilibrium points in the generalised photogravitational elliptic restricted three-body problemen
dc.typeArticleen
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