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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2854
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dc.contributor.authorGiridhar, S-
dc.contributor.authorKameswara Rao, N-
dc.contributor.authorLambert, D. L-
dc.date.accessioned2008-07-23T11:28:19Z-
dc.date.available2008-07-23T11:28:19Z-
dc.date.issued1996-06-
dc.identifier.citationJournal of Astrophysics and Astronomy, Vol. 17, No. 1 - 2, pp. 23 - 40en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2248/2854-
dc.description.abstractTwo high resolution spectra of the hot RCrB star DY Cen in the red region are compared. The photospheric absorption lines show a radial velocity variation of 12 km s(sup -1) between 1989 July and 1992 May. Emission components to some CII lines present in 1989 are almost entirely absent in 1992. Nebular forbidden lines of [OI], [NII] and [SII] appear unchanged from 1989 to 1992.en
dc.format.extent1008774 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndaian Academy of Sciencesen
dc.relation.urihttp://adsabs.harvard.edu/abs/1996JApA...17...23Gen
dc.subjectHot RCrB starsen
dc.subjectRadial velocityen
dc.subjectPhotospheric and nebular linesen
dc.titleSpectral Variations of DY Cenen
dc.typeArticleen
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