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Photometry of Zeta Aurigae during the 1977 and 1979-80 Eclipses

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dc.contributor.author Mohin, S
dc.contributor.author Raveendran, A. V
dc.contributor.author Mekkaden, M. V
dc.date.accessioned 2005-03-02T06:19:54Z
dc.date.available 2005-03-02T06:19:54Z
dc.date.issued 1980
dc.identifier.citation Kodaikanal Observatory Bulletins Series A, Vol. 3, pp. 1-5 en
dc.identifier.issn 0374-3632
dc.identifier.uri http://hdl.handle.net/2248/371
dc.description.abstract UBV photometry of Zeta Aurigae during the 1977 and 1979-80 eclipses is presented. From an analysis of the available photometry, it is concluded that the long term intrinsic variation in the brightness of the late-type super giant companion, as claimed by various investigators, is far from certain. en
dc.format.extent 141925 bytes
dc.format.mimetype application/pdf
dc.language.iso en
dc.publisher Indian Institute of Astrophysics, Bangalore en
dc.subject Eclipsing binaries en
dc.subject Zeta Aurigae en
dc.subject UBV Photometry en
dc.subject Variable Stars en
dc.title Photometry of Zeta Aurigae during the 1977 and 1979-80 Eclipses en
dc.type Article en


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