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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6771
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dc.contributor.authorHema, B. P-
dc.contributor.authorPandey, G-
dc.contributor.authorKamath, D-
dc.contributor.authorKameswara Rao, N-
dc.contributor.authorLambert, D. L-
dc.contributor.authorWoolf, V. M-
dc.date.accessioned2020-11-10T13:32:51Z-
dc.date.available2020-11-10T13:32:51Z-
dc.date.issued2017-10-
dc.identifier.citationPublications of the Astronomical Society of the Pacific, Vol. 129, No. 980, 104202en_US
dc.identifier.issn0004-6280-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6771-
dc.descriptionRestricted Access © The Astronomical Society of the Pacific https://doi.org/10.1088/1538-3873/aa7f25en_US
dc.description.abstractAbundance analyses of the two newly discovered R Coronae Borealis (RCB) stars ASAS-RCB-8 and ASAS-RCB-10 were conducted using high-resolution optical spectra and model atmospheres. Their chemical compositions place the pair among the majority class of RCBs. ASAS-RCB-10 is one of the most N-poor majority RCBs with an above average O abundance. Relative to ASAS-RCB-10, ASAS-RCB-8 is H poor by 1.6 dex, O-poor by 0.7 dex but N-rich by 0.8 dex suggesting a higher contamination by CNO-cycled material.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.subjectStars: abundancesen_US
dc.subjectStars: chemically peculiaren_US
dc.subjectStars: distancesen_US
dc.titleAbundance Analyses of the New R Coronae Borealis Stars ASAS-RCB-8 and ASAS-RCB-10en_US
dc.typeArticleen_US
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