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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3823
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dc.contributor.authorShylaja, B. S-
dc.date.accessioned2008-09-23T13:46:16Z-
dc.date.available2008-09-23T13:46:16Z-
dc.date.issued1987-06-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 8, No. 2, pp. 183 - 194.en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3823-
dc.description.abstractThe behaviour of the λ4686 line of He II in various WN binaries is studied for variations in total flux as well as radial velocities. It appears that the true motion of the WN component is not depicted by this line especially for short-period binaries. A qualitative explanation is sought in terms of a large, extended line-emitting region and multiple-component line profile.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1987JApA....8..183Sen
dc.subjectBinary starsen
dc.subjectLine spectraen
dc.subjectStellar spectraen
dc.subjectAstronomical catalogsen
dc.subjectFlux quantizationen
dc.subjectheliumen
dc.subjectRadial velocityen
dc.titleThe He II line 4686 in WN binariesen
dc.typeArticleen
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