Eclipsing binary signatures in Zeta Capricorni

dc.contributor.author	Srivastava, R. K.
dc.date.accessioned	2010-02-17T06:56:10Z
dc.date.available	2010-02-17T06:56:10Z
dc.date.issued	1988
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/534
dc.description.abstract	Zeta Capricorni (ζ Cap HD 204075) was shown to be a Barium line spectroscopic binary, possessing strong BaII line by Bohm-Vitense (1980), Smith et al.(1980), Culiver (1981) and Smith and Lambert (1984). ζ Cap is shown to have a white dwarf companion by Bohm-Vitense (1980), which is much fainter than ζ Cap. Photoelectric observations of ζ Cap. Photoelectric observations of ζ Cap are hardly available in the literature except for the color indices (B-V=1.ͫ00 and U-B=0.ͫ59, Sp.=G5) given by Eggen (1972).	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	abvs3217
dc.subject	Zeta Capricorni	en_US
dc.title	Eclipsing binary signatures in Zeta Capricorni	en_US
dc.type	Article	en_US