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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3877
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dc.contributor.authorShylaja, B. S-
dc.date.accessioned2008-09-24T14:38:28Z-
dc.date.available2008-09-24T14:38:28Z-
dc.date.issued1986-12-
dc.identifier.citationJournal of Astrophysics and Astronomy , Vol. 7, No. 4, pp. 305 - 316en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/3877-
dc.description.abstractNew spectrophotometric observations of the Wolf-Rayet system HD 50896 are presented and interpreted in terms of its binary nature. The lines of N V, N IV and C IV show moderate variations which can be explained using a binary model with a compact companion. The He II 4686A line appears to arise from a larger region than other lines. The distortion caused by the wind can partly explain its flux variations. The emission fluxes of He I lines are generally constant, indicating their nonparticipation in the orbit. The results are compared with other Wolf-Rayet binaries (V444 Cyg and CQ Cep) and the evolutionary status is discussed.en
dc.language.isoenen
dc.publisherIndian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1986JApA....7..305Sen
dc.subjectBinary starsen
dc.subjectSpectrum analysisen
dc.subjectStellar spectrophotometryen
dc.subjectWolf-rayet starsen
dc.subjectAbundanceen
dc.subjectEmission spectraen
dc.subjectLine spectraen
dc.subjectRadiant flux densityen
dc.subjectStellar windsen
dc.titleA spectrophotometric study of the Wolf-Rayet star HD 50896en
dc.typeArticleen
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