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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4251
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dc.contributor.authorGhosh, K. K-
dc.date.accessioned2009-01-07T12:39:22Z-
dc.date.available2009-01-07T12:39:22Z-
dc.date.issued1988-08-
dc.identifier.citationAstrophysics and Space Science, Vol. 147, No. 1, pp. 91 - 106en
dc.identifier.issn0004-640X-
dc.identifier.urihttp://hdl.handle.net/2248/4251-
dc.description.abstractRapid observations of H profiles of eight Be stars have been obtained and it is found that rapid (in a time-scale of 4 to 6 minutes) and irregular variations of total emission strength of H line are present in these stars. It has been suggested that these variations may be due to the material circulation in the envelope of Be stars.en
dc.language.isoenen
dc.publisherKluwer Academic Publishersen
dc.relation.urihttp://dx.doi.org/10.1007/BF00656609en
dc.relation.urihttp://adsabs.harvard.edu/abs/1988Ap%26SS.147...91Gen
dc.subjectB Starsen
dc.subjectEmission Spectraen
dc.subjectH Alpha Lineen
dc.subjectStellar Spectraen
dc.subjectAstronomical Catalogsen
dc.subjectPhotoelectronsen
dc.subjectStellar Envelopesen
dc.subjectVisible Spectrumen
dc.titleRapid variations of H-alpha emission strength of eight Be starsen
dc.typeArticleen
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