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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1430
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dc.contributor.authorKameswara Rao, N-
dc.date.accessioned2007-03-14T08:43:50Z-
dc.date.available2007-03-14T08:43:50Z-
dc.date.issued1990-
dc.identifier.citationBASI, Vol. 18, pp. 341-350en
dc.identifier.urihttp://hdl.handle.net/2248/1430-
dc.description.abstractThe properties of the hydrogen-deficient stars called extreme helium stars, R Cr B stars, and hydrogen-deficient carbon stars are briefly examined, emphasizing the R Cr B stars. Luminosities and temperatures, distribution and kinematics, abundances, pulsations, circumstellar environment, and structure and origin are addressed. The stage of stellar evolution at which a medium-mass star of normal composition could become hydrogen-deficient is considered.en
dc.format.extent301591 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectStellar evolutionen
dc.subjectVariable staren
dc.titleThe evolutionary considerations of R CR B stars - Observational approachen
dc.typeArticleen
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