UBV photometry of DX Aquarii

dc.contributor.author	Srivastava, R. K.
dc.contributor.author	Sinha, B. K.
dc.date.accessioned	2010-03-03T10:54:06Z
dc.date.available	2010-03-03T10:54:06Z
dc.date.issued	1985
dc.identifier.citation	This article is downloaded from ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/604
dc.description.abstract	U, B, V photometry of the Eclipsing binary system DX Aqr has been presented for the first time. The period of the system comes out to be nearly half the period given by Strohmeier (1966) and a value of 0ͩ.472502 has been determined. The colour of the system has been discussed. The primaru eclipse is a total occulation. The orbit seems to be eccentric. The system belongs to Algol type. DX Aqr may be a very complicated system. The present results are considerably different from those of earlier investigations.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass111-225
dc.subject	Eclipsing binary system DX Aquarii	en_US
dc.title	UBV photometry of DX Aquarii	en_US
dc.type	Article	en_US