HD 126200 - a suspected eclipsing binary?

dc.contributor.author	Srivastava, J. B.
dc.contributor.author	Kandpal, C. D.
dc.date.accessioned	2010-03-09T06:41:29Z
dc.date.available	2010-03-09T06:41:29Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/620
dc.description.abstract	The star HD 126200 (= BD+8°2857) has now been listed by Kukarkin et al. (1982) as a suspected eclipsing binary of Algol type with a variation of 0.5 magnitude based on the findings of Sanding (1951). Hirschfeld and Sinnott (1982) have listed its magnitude, colour, radial velocity and spectral type. No other information about the star is available in the literature.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs2574
dc.subject	Eclipsing binary HD 126200	en_US
dc.title	HD 126200 - a suspected eclipsing binary?	en_US
dc.type	Article	en_US