Photometric study of the short period W UMa system - FZ Orionis

dc.contributor.author	Rukmini, J
dc.contributor.author	Vivekananda Rao, P
dc.contributor.author	Ausekar, B. D
dc.date.accessioned	2008-05-08T09:40:05Z
dc.date.available	2008-05-08T09:40:05Z
dc.date.issued	2001
dc.identifier.citation	BASI, Vol. 29, No. 3, pp. 323 - 327	en
dc.identifier.uri	http://hdl.handle.net/2248/2274
dc.description.abstract	Photoelectric B, V observations of the eclipsing binary system FZ Orionis obtained from the Japal-Rangapur Observatory during the years 1981 to 1992 are presented and studied. No period changes in the system are detected. The light curves are analysed using the Wilson-Devinney method and the system parameters are derived.	en
dc.format.extent	355475 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2001BASI...29..323R	en
dc.subject	Photoelectric	en
dc.subject	W UMa system	en
dc.subject	FZ Orionis	en
dc.title	Photometric study of the short period W UMa system - FZ Orionis	en
dc.type	Article	en