Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4252
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dc.contributor.authorGhosh, K. K-
dc.contributor.authorSanjeevkumar, T-
dc.contributor.authorJaykumar, K-
dc.contributor.authorKuppuswamy, K-
dc.contributor.authorRosario, M. J-
dc.date.accessioned2009-01-07T12:40:44Z-
dc.date.available2009-01-07T12:40:44Z-
dc.date.issued1988-06-
dc.identifier.citationPublications Astronomical Society of the Pacific, Vol. 100, pp. 719 - 723en
dc.identifier.issn0004-6280-
dc.identifier.urihttp://hdl.handle.net/2248/4252-
dc.description.abstractA search for rapid variability of H-alpha with a time resolution from 30 to 45 seconds is performed for Phi Per. In total, 42 spectra in H-alpha were obtained during three nights. Results show the presence of rapid irregular variability (time scale of a few minutes) of the equivalent width of the H-alpha line in Phi Per.en
dc.language.isoenen
dc.publisherAstronomical Society of the Pacificen
dc.relation.urihttp://adsabs.harvard.edu/abs/1988PASP..100..719Gen
dc.relation.urihttp://dx.doi.org/10.1086/132225en
dc.subjectB Starsen
dc.subjectEmission Spectraen
dc.subjectH Alpha Lineen
dc.subjectLine Shapeen
dc.subjectVariabilityen
dc.subjectBalmer Seriesen
dc.subjectStellar Rotationen
dc.titleRapid H-alpha variability in Phi Perseien
dc.typeArticleen
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