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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/349
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dc.contributor.authorAbhyankar, K. D-
dc.contributor.authorPanchatsaram, T-
dc.date.accessioned2005-02-09T06:11:31Z-
dc.date.available2005-02-09T06:11:31Z-
dc.date.issued1982-12-
dc.identifier.citationBASI, Vol. 10, No. 4, pp. 315-322en
dc.identifier.urihttp://hdl.handle.net/2248/349-
dc.description.abstractAn analysis of the minimum-time data of AK Her and ER Ori revelas possible sinudodal variations in their orbital periods. In the case of AK Her we suspect two additional components; one of mass 0.2 to 0.4 MSun with a period of 62 yr and the other of mass 0.2 to 0.6 MSun with a period of 207 yr. The probable third mass in ER Ori is less than 0.6 MSun for i>or equal to 60 degree with a long-term period of 34.78 yr.en
dc.format.extent586715 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectAK Heren
dc.subjectER Orien
dc.subjectminimum-time dataen
dc.titleLight-time effect in AK Her and ER Orien
dc.typeArticleen
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