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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4321
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dc.contributor.authorRajamohan, R-
dc.date.accessioned2009-02-04T16:07:56Z-
dc.date.available2009-02-04T16:07:56Z-
dc.date.issued1984-02-
dc.identifier.citationAstrophysics and Space Science, Vol. 99, No. 1 - 2, pp. 153 - 155en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4321-
dc.description.abstractA brief description of the variation of the Hα line profile in γ Velorum and HD 47129 is given.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://adsabs.harvard.edu/abs/1984Ap%26SS..99..153Ren
dc.relation.urihttp://www.springerlink.com/content/p1v078r1k6741k76/en
dc.subjectBinary Starsen
dc.subjectEarly Starsen
dc.subjectH Alpha Lineen
dc.subjectWolf-Rayet Starsen
dc.subjectEmission Spectraen
dc.subjectRadial Velocityen
dc.subjectSpectral Energy Distributionen
dc.subjectStellar Spectrophotometryen
dc.titleThe H-alpha line profile in early type-binary systems HD 47129 and Gamma Velorumen
dc.typeArticleen
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