Photometric study of BZ Eridani

dc.contributor.author	Srivastava, R. K.
dc.contributor.author	Uddin, W.
dc.date.accessioned	2010-02-22T05:39:45Z
dc.date.available	2010-02-22T05:39:45Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/560
dc.description.abstract	The 1980-1981 U, B and V observations of the eclipsing binary BZ Eridani have been presented. A new period of BZ Eri comes out to be 0. ͩ 6641703. The colour curves of the system show appreciable variations, and are indicative of intrinsic variability. The secondary minimum falls nearly at phase 0.5. Some interesting features are given. The features of BZ Eri are changing. Some light variations are visible around the p[hase of secondary minimum. The discussion reveals that BZ Eri is a complicated system.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	apss126-105
dc.subject	BZ Eridani	en_US
dc.title	Photometric study of BZ Eridani	en_US
dc.type	Article	en_US