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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2237
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dc.contributor.authorStoica, C-
dc.contributor.authorMioc, V-
dc.date.accessioned2008-04-21T10:02:07Z-
dc.date.available2008-04-21T10:02:07Z-
dc.date.issued1997-
dc.identifier.citationBASI, Vol. 25, No. 2, pp. 217 - 225en
dc.identifier.urihttp://hdl.handle.net/2248/2237-
dc.description.abstractA qualitative study of the two-body problem in Maneff's gravitational field is being performed by representing the motion in the (1/r, r-plane. The phase trajectories are found to be only conic sections(or arcs of them). Each allowed trajectory is interpreted from the standpoint of physical motion. Concrete astronomical exemplifications are made.en
dc.format.extent732442 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1997BASI...25..217Sen
dc.subjectCelestial Mechanicsen
dc.subjectManeff's Fielden
dc.subjectQualitative Theoryen
dc.titleGeometrical and physical description of the two-body problem in Maneff's gravitational fielden
dc.typeArticleen
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