Flare like activities in eclipsing binary DI Peg

dc.contributor.author	Chaubey, U. S.
dc.date.accessioned	2011-01-10T06:59:43Z
dc.date.available	2011-01-10T06:59:43Z
dc.date.issued	1980
dc.identifier.citation	This article is taken from ADS database	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/772
dc.description.abstract	The eclipsing binary DI Peg (BD+14d5006, HD 220619) was selected for UBV photometry because earlier photometric investigations drew attention to its interesting nature (Jensch, 1934, Rucinski, 1967 and Binnendijk, 1973). Rucinski (1967) derived an orbital solution by assuming 24% extra light in V light.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs1739
dc.subject	DI Peg - eclipsing binary	en_US
dc.title	Flare like activities in eclipsing binary DI Peg	en_US
dc.type	Article	en_US