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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/311
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dc.contributor.authorPanchatsaram, T-
dc.date.accessioned2005-02-04T16:14:44Z-
dc.date.available2005-02-04T16:14:44Z-
dc.date.issued1981-06-
dc.identifier.citationBASI, Vol. 9, No. 2, pp. 139-143en
dc.identifier.urihttp://hdl.handle.net/2248/311-
dc.description.abstractWith the available photoelectric times of minima the variations in the orbital period of U Oph can be interpreted in terms of the presence of a third body.en
dc.format.extent327355 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjecteclipsing binariesen
dc.subjectperiod changesen
dc.subjectlight time effecten
dc.titleA study of the period of U Ophiuchien
dc.typeArticleen
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