Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/77
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBappu, M. K. V-
dc.contributor.authorVisvanadham, P-
dc.date.accessioned2004-12-01T06:51:23Z-
dc.date.available2004-12-01T06:51:23Z-
dc.date.issued1977-
dc.identifier.citationKodaikanal Observatory Bulletins Series A, Vol. 2, pp. 89-94en
dc.identifier.issn0374-3632-
dc.identifier.urihttp://hdl.handle.net/2248/77-
dc.description.abstractVelocity curves of the system HD 214419 are obtained for the N IV 4058 and He II 4686 emission lines from prismatic spectra taken in 1951 and 1952. The emission and absorption features experience several phase dependent changes that are described in detail. A common envelope model expalins well the He II 4686 light and velocity changes. The system parameters are best derived from N IV 4058.en
dc.format.extent564363 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherIndian Institute of Astrophysics, Bangaloreen
dc.subjectCQ Cepheien
dc.subjectWolf-Rayet Staren
dc.subjectVelocity Curveen
dc.subjectSpectral Changesen
dc.titleThe Wolf-Rayet Spectrscopic Binary HD 214419en
dc.typeArticleen
Appears in Collections:IIAP Publications
Kodaikanal Observatory Bulletins (1905 - 1997 )
M.K. Vainu Bappu ( 1960 - 1982 )

Files in This Item:
File Description SizeFormat 
The Wolf-Rayet Spectrscopic Binary HD 214419.pdf551.14 kBAdobe PDFThumbnail
View/Open


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.