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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3769
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dc.contributor.authorGiridhar, S-
dc.date.accessioned2008-09-22T12:09:01Z-
dc.date.available2008-09-22T12:09:01Z-
dc.date.issued1987-05-
dc.identifier.citationRevista Mexicana de Astronomia y Astrofisica , Vol. 14, No. 2, pp. 431 - 434en
dc.identifier.issn0185-1101-
dc.identifier.urihttp://hdl.handle.net/2248/3769-
dc.description.abstractFine analysis of the southern Cepheid β Dor has been conducted at different phases with the aim to derive atmospheric parameters at those phases. Atmospheric abundances have been derived for Fe group elements and s-process elements. The derived parameters of β Dor are compared with earlier estimates.en
dc.language.isoenen
dc.publisherUniversidad Nacional Autonoma De Mexicoen
dc.relation.urihttp://adsabs.harvard.edu/abs/1987RMxAA..14..431Gen
dc.subjectStar Abundanceen
dc.subjectCepheid variablesen
dc.subjectStellar atmospheresen
dc.subjectStellar spectraen
dc.subjectAtmospheric modelsen
dc.subjectElectron scatteringen
dc.subjectLine spectraen
dc.titleSpectroscopic studies of the southern Cepheid β Doren
dc.typeArticleen
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