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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2637
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dc.contributor.authorGhosh, K. K-
dc.date.accessioned2008-07-11T10:19:37Z-
dc.date.available2008-07-11T10:19:37Z-
dc.date.issued1994-
dc.identifier.citationIAU Symposium, No. 162, pp. 351 – 353en
dc.identifier.issn0074-1809-
dc.identifier.urihttp://hdl.handle.net/2248/2637-
dc.description.abstractBased on Spectrosopic observations of more than 100 Be stars, we present the reuslts of the phase changes of Be stars.en
dc.format.extent193182 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherInternational Astronomical Unionen
dc.relation.urihttp://adsabs.harvard.edu/abs/1994IAUS..162..351Gen
dc.subjectBe starsen
dc.subjectPhysicsen
dc.subjectSpectrosopic observationsen
dc.titlePhysics of the phase changes of Be starsen
dc.typeArticleen
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