Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7188
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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.accessioned2017-10-09T10:52:25Z-
dc.date.available2017-10-09T10:52:25Z-
dc.date.issued2017-10-01-
dc.identifier.citationPublications of the Astronomical Society of the Pacific, Vol. 129, No. 980, 104202en_US
dc.identifier.issn0004-6280-
dc.identifier.urihttp://hdl.handle.net/2248/7188-
dc.descriptionRestricted Accessen_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 Publishing on behalf of the Astronomical Society of the Pacificen_US
dc.relation.urihttps://doi.org/10.1088/1538-3873/aa7f25-
dc.rights© The Astronomical Society of the Pacific-
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
Appears in Collections:IIAP Publications

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