Photoelectric study of AW UMa

dc.contributor.author	Sridharan, R. K.
dc.contributor.author	Padalia, T. D.
dc.date.accessioned	2010-02-08T08:49:12Z
dc.date.available	2010-02-08T08:49:12Z
dc.date.issued	1986
dc.identifier.uri	http://hdl.handle.net/123456789/492
dc.description.abstract	UBV photoelectric photometry of the eclipsing binary system AW UMa has been presented. A slightly improved period of 0 ͩ.4387304 has been given. The colour of the system has been discussed. Eccentricity is present in the system. Light and colour curves show that intrinsic light variations may be present of the system. The presence of mass transfer is a possibility.	en_US
dc.language.iso	en	en_US
dc.relation.ispartofseries	apss120-121
dc.subject	Photoelectric, Photometry	en_US
dc.title	Photoelectric study of AW UMa	en_US
dc.type	Article	en_US