Variability of the Hα emissions in ϕ Per

dc.contributor.author	Goraya, P. S.
dc.date.accessioned	2010-03-09T06:09:40Z
dc.date.available	2010-03-09T06:09:40Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/619
dc.description.abstract	Photoelectric scans of the Be shell star ϕ Per in the Hα region have been taken to investigate the variations of Hα emission lines. Definite variations with time-scale of a few minutes have been detected. It is hoped that hydromagnetic instability within the envelop is responsible for such variations.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ass107-323
dc.subject	Be shell star ϕ Per	en_US
dc.title	Variability of the Hα emissions in ϕ Per	en_US
dc.type	Article	en_US