The RS Canum Venaticorum binary HD 116204

dc.contributor.author	Mohin, S
dc.contributor.author	Raveendran, A. V
dc.date.accessioned	2008-09-22T11:36:06Z
dc.date.available	2008-09-22T11:36:06Z
dc.date.issued	1987-12
dc.identifier.citation	Journal of Astrophysics and Astronomy , Vol. 8, No. 4, pp. 389 - 395	en
dc.identifier.issn	0250-6335
dc.identifier.uri	http://hdl.handle.net/2248/3757
dc.description.abstract	BV photometry of HD 116204 have been obtained on 57 nights during the 1983-1984, 1984-1985, and 1986-1987 observing seasons with the 34-cm reflector of the Vainu Bappu Observatory in Kavalur. A photometric period of 21.9 + or - 0.2 d and a mean (B-V) of 1.196 + or - 0.010 have been determined, and a mass ratio close to unity for HD 116204 is implied. The results suggest a vertical shift of the entire light curve towards brighter magnitudes and a low inclination of the rotation axis.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1987JApA....8..389M	en
dc.subject	Binary stars	en
dc.subject	Stellar spectrophotometry	en
dc.subject	UBV spectra	en
dc.subject	Visual photometry	en
dc.subject	Light curve	en
dc.subject	Mass ratios	en
dc.subject	Stellar color	en
dc.subject	Stellar magnitude	en
dc.subject	Stellar mass	en
dc.subject	BV Photometry	en
dc.subject	HD116204	en
dc.subject	RS CVn System	en
dc.title	The RS Canum Venaticorum binary HD 116204	en
dc.type	Article	en