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

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/371

Full metadata record

DC Field	Value	Language
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
Appears in Collections:	IIAP Publications Kodaikanal Observatory Bulletins (1905 - 1997 )

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