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dc.contributor.authorRaghubar Singh-
dc.contributor.authorBharat Kumar, Y-
dc.contributor.authorReddy, B. E-
dc.contributor.authorAoki, W-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 491, No. 3, pp. 3838–3843en_US
dc.descriptionRestricted Accessen_US
dc.description.abstractGiven the implications for the origin of Li enhancement in red giants, we have reviewed the Li-rich classification of KIC 9821622, the only bonafide red giant branch (RGB) giant with a He inert core to date, reported as a Li-rich giant by reanalysing the high-resolution spectra. We have obtained A(Li)LTE = 1.42 ± 0.05 dex. After correcting for non-local thermodynamic equilibrium (NLTE), we have A(Li)NLTE = 1.57 ± 0.05 dex, which is significantly less than the reported A(Li) = 1.80 ± 0.2 dex. We found that the subordinate line at 6103 Å is too weak or absent to measure Li abundance. The derived abundance is normal for red giants undergoing dilution during the first dredge-up. Since all known Kepler field Li-rich giants belong to the red clump region, this clarification removes the anomaly and strengthens the evidence that Li enhancement in low-mass giants may be associated only with the He-core burning phase. The origin of Li excess probably lies during the He flash at the RGB tip, a phase immediately preceding the red clump.en_US
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
dc.rights© Royal Astronomical Society-
dc.subjectStars: abundancesen_US
dc.subjectStars: evolutionen_US
dc.subjectStars: fundamental parameters,en_US
dc.subjectStars: low-massen_US
dc.titleConcerning the Li-rich status of KIC 9821622: a Kepler field RGB star reported as a Li-rich gianten_US
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