Analysis of the light variations of BS Aquarii

dc.contributor.author	Kilambi, G. C
dc.date.accessioned	2005-02-09T04:30:34Z
dc.date.available	2005-02-09T04:30:34Z
dc.date.issued	1982-09
dc.identifier.citation	BASI, Vol. 10, No. 3, pp. 234-243	en
dc.identifier.uri	http://hdl.handle.net/2248/345
dc.description.abstract	An analysis of UBV light variations of BS Aqr is presented. Intrinsic (U-B) and (B-V) values are used to derive the temperature and surface gravity. The mean values are Teff = 7600 + or - 100 K and log geff = 3.8 + or - 0.1. These values suggest that BS Aqr is a normal population I pulsating star and a member of Delta-Scuti group.	en
dc.format.extent	709799 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en
dc.publisher	Astronomical Society of India	en
dc.subject	variable star	en
dc.subject	photometry	en
dc.subject	pulsation	en
dc.subject	dwarf Cepheid	en
dc.title	Analysis of the light variations of BS Aquarii	en
dc.type	Article	en