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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4365
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dc.contributor.authorRaveendran, A. V-
dc.contributor.authorAshoka, B. N-
dc.contributor.authorKameswara Rao, N-
dc.date.accessioned2009-03-03T09:27:17Z-
dc.date.available2009-03-03T09:27:17Z-
dc.date.issued1986-
dc.identifier.citationKurt Hunger, Detlef Schoenberner, and N. Kameswara Rao., eds., Hydrogen Deficient Stars and Related Objects, Proceedings of IAU Colloq. 87, held in Mysore, India, Nov. 10 - 15, 1985, Vol. 128, pp. 191 - 195en
dc.identifier.urihttp://hdl.handle.net/2248/4365-
dc.description.abstractFourier analysis of the light curves of R CrB in the V band near maximum shows that in addition to several significant short periods there is a modulation of the visual light with a period around 1170 days, similar to that of the L band flux, noticed by Strecker. This indicates that there is some contribution to the visual light variations of the star from the pulsating circumstellar dust. Radial velocities of R CrB obtained at Kavalur during February-May 1985 show variations with a period around 47 days.en
dc.language.isoenen
dc.publisherD. Reidel Publishing Coen
dc.relation.urihttp://adsabs.harvard.edu/abs/1986ASSL..128..191Ren
dc.subjectLight Curveen
dc.subjectRadial Velocityen
dc.subjectRadiant Flux Densityen
dc.subjectStellar Spectrophotometryen
dc.subjectVariable Starsen
dc.subjectFourier Analysisen
dc.subjectPower Spectraen
dc.subjectStellar Envelopesen
dc.subjectUBV Spectraen
dc.titlePhotometric and radial velocity variations of RCrB near maximum lighten
dc.typeArticleen
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