Photoelctric photometry of the eclipsing binary EE Aqr

dc.contributor.author	Padalia, T. D.
dc.date.accessioned	2011-11-09T04:55:30Z
dc.date.available	2011-11-09T04:55:30Z
dc.date.issued	1979
dc.identifier.citation	This article is downloaded from ADS article services	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/857
dc.description.abstract	The system EE Aqr has been observed in UBV colours. A consistent set of orbital elements and a slightly improved period of 0.ᵈ5089954 have been obtained. The eclipse is partial and varability is of β Lyrae-type. The colour of the components has been determined.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass62-477
dc.subject	Eclipsing Binary EE Aqr	en_US
dc.title	Photoelctric photometry of the eclipsing binary EE Aqr	en_US
dc.type	Article	en_US