Variable line strengths of star HD 50896

dc.contributor.author	Singh, M.
dc.date.accessioned	2010-03-10T08:37:21Z
dc.date.available	2010-03-10T08:37:21Z
dc.date.issued	1984
dc.identifier.citation	This article is downloaded for ADS	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/634
dc.description.abstract	Wolf-Rayet stars from a distinct class of stellar objects and have spectra in which emission lines of either nitrogen and helium predominate (WN) or else emission lines of helium, carbon and oxygen predominate (WC). Furthermore, these stars suffer mass loss through strong stellar winds. Their evolutionary status is also of significant interest since these objects are suspected to be supernovae precursors.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	ibvs2508
dc.subject	Star HD 50896	en_US
dc.title	Variable line strengths of star HD 50896	en_US
dc.type	Article	en_US