Hα  variability in alpha lyrae

dc.contributor.author	Goraya, P. S.
dc.contributor.author	Singh, M.
dc.date.accessioned	2010-03-09T06:47:31Z
dc.date.available	2010-03-09T06:47:31Z
dc.date.issued	1983
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/621
dc.description.abstract	Suspected variability is a valuable clue in finding new emission stars. Hα observations of bright stars with no history of line emission can lead to the discovery of hydrogen-emission stars. α Lyrae had been a well known standard star with spectral type AOV.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs2455
dc.subject	New emission stars - Hydrogen emission stars, Alpha lyrae	en_US
dc.title	Hα variability in alpha lyrae	en_US
dc.type	Article	en_US