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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/305
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dc.contributor.authorPanchatsaram, T-
dc.contributor.authorAbhyankar, K. D-
dc.date.accessioned2005-02-04T15:36:05Z-
dc.date.available2005-02-04T15:36:05Z-
dc.date.issued1981-03-
dc.identifier.citationBASI, Vol. 9, No. 1, pp. 31-39en
dc.identifier.urihttp://hdl.handle.net/2248/305-
dc.description.abstractOrbital period study using photoelectric times of minima of SW Lac revelas that the period change is caused by the orbital motion of a triple system around a fourth body. The orbital periods of the third and the fourth body are 19.67 yr and 70.25 respectively, and their masses are close to 1 M Radius each.en
dc.format.extent638598 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectSW Lacen
dc.subjectmultiple star systemsen
dc.titleSW Lacertae - A quadruple systemen
dc.typeArticleen
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