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Light-time effect in AK Her and ER Ori

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dc.contributor.author Abhyankar, K. D
dc.contributor.author Panchatsaram, T
dc.date.accessioned 2005-02-09T06:11:31Z
dc.date.available 2005-02-09T06:11:31Z
dc.date.issued 1982-12
dc.identifier.citation BASI, Vol. 10, No. 4, pp. 315-322 en
dc.identifier.uri http://hdl.handle.net/2248/349
dc.description.abstract An 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.extent 586715 bytes
dc.format.mimetype application/pdf
dc.language.iso en
dc.publisher Astronomical Society of India en
dc.subject AK Her en
dc.subject ER Ori en
dc.subject minimum-time data en
dc.title Light-time effect in AK Her and ER Ori en
dc.type Article en


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