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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2109
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dc.contributor.authorPandey, G-
dc.contributor.authorKameswara Rao, N-
dc.contributor.authorLambert, D. L-
dc.contributor.authorJeffery, C. S-
dc.contributor.authorAsplund, M-
dc.date.accessioned2008-03-03T10:17:10Z-
dc.date.available2008-03-03T10:17:10Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 303 - 304en
dc.identifier.urihttp://hdl.handle.net/2248/2109-
dc.description.abstractHigh resolution spectra were obtained for a sample of hydrogen-deficient stars which are hotter than the R CrB stars and cooler among the extreme helium stars (EHe). We believe that these stars are transition objects evolving either to EHe stars or R CrB stars. We aim to explore the evolutionary link between our program stars, R CrB stars and EHe stars. Distribution of these stars in the log g - log Teff plane shows similar L/M ratios (≈4.0). These objects have an abundance pattern like R CrB stars and EHe stars.en
dc.format.extent156920 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..303Pen
dc.subjectEHe starsen
dc.subjectAbundanceen
dc.subjectStellar evolutionen
dc.titleAbundance analysis of extreme helium starsen
dc.typeArticleen
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