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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1908
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dc.contributor.authorGoswami, A-
dc.contributor.authorKameswara Rao, N-
dc.contributor.authorLambert, D. L-
dc.date.accessioned2007-10-19T09:13:47Z-
dc.date.available2007-10-19T09:13:47Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 129 - 132en
dc.identifier.urihttp://hdl.handle.net/2248/1908-
dc.description.abstractThe analysis of high-resolution spectra of DZ Andromedae, a suspected R Coronae Borealis variable, is presented here. The spectra of DZ And show the characteristics of a normal K2 III star, indicating that the star was earlier misclassifed. A detailed abundance analysis also indicates that the star's composition is not consistent with its membership in the RCB class.en
dc.format.extent214190 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..129Gen
dc.subjectDZ Andromedaeen
dc.subjectRCB starsen
dc.titleDZ Andromedae : A search for the spectral evidence of its possible RCB natureen
dc.typeArticleen
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