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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1886
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dc.contributor.authorAhmad, A-
dc.contributor.authorIslam, N-
dc.date.accessioned2007-10-16T06:00:53Z-
dc.date.available2007-10-16T06:00:53Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 1, pp. 83 - 86en
dc.identifier.urihttp://hdl.handle.net/2248/1886-
dc.description.abstractHere, we have deduced the equations of motion of the photogravitional restricted three-body problem considering the effect of solar radiation pressure on a planet and found that it is stabilizing for the triangular libration points.en
dc.format.extent213600 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25...83Aen
dc.subjectPhotogravitionalen
dc.subjectLagrangianen
dc.subjectThree-bodyen
dc.titleEffect of solar radiation pressure on a planet in the photogravitational restricted three-body problemen
dc.typeArticleen
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