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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/617
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dc.contributor.authorHirata, Ryuko-
dc.contributor.authorKogure, T-
dc.date.accessioned2005-12-06T08:56:34Z-
dc.date.available2005-12-06T08:56:34Z-
dc.date.issued1984-06-
dc.identifier.citationBASI, Vol. 12, No. 2, pp. 109-151en
dc.identifier.urihttp://hdl.handle.net/2248/617-
dc.format.extent4123136 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoen-
dc.publisherAstronomical Society of Indiaen
dc.subjectBe starsen
dc.subjectShell starsen
dc.subjectContinuous spectrumen
dc.subjectEmission linesen
dc.subjectShell absorption linesen
dc.subjectCool envelopesen
dc.subjectHot regionsen
dc.titleThe Be star phenomena II. Spectral formation and structure of envelopesen
dc.typeArticleen
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