Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3806
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dc.contributor.authorShylaja, B. S-
dc.date.accessioned2008-09-23T10:49:55Z-
dc.date.available2008-09-23T10:49:55Z-
dc.date.issued1987-
dc.identifier.citationIAU Symposium, No. 122, pp. 459 - 460en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/3806-
dc.description.abstractThe binaries with subgroup WN components have been chosen, with periods ranging from 1.64 d to 21.63 d, for understanding the effect of the companion on the formation of this line.en
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://ads.ari.uni-heidelberg.de/abs/1987IAUS..122..459Sen
dc.subjectBinaries:wolf-rayet starsen
dc.subjectWolf-Rayet Stars:binariesen
dc.titleThe behaviour of λ4686 line of He II in Wolf-Rayet binariesen
dc.typeArticleen
Appears in Collections:IIAP Publications

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