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• W2108571343 startingPage "L94" @default.
• W2108571343 abstract "An analysis of the fluorine abundance in Galactic asymptotic giant branch (AGB) carbon stars (24 N-type, 5 SC-type, and 5 J-type) is presented. This study uses the state-of-the-art carbon-rich atmosphere models and improved atomic and molecular line lists in the 2.3 μm region. Significantly lower F abundances are obtained in comparison to previous studies in the literature. This difference is mainly due to molecular blends. In the case of carbon stars of SC-type, differences in the model atmospheres are also relevant. The new F enhancements are now in agreement with the most recent theoretical nucleosynthesis models in low-mass AGB stars, solving the long-standing problem of F in Galactic AGB stars. Nevertheless, some SC-type carbon stars still show larger F abundances than predicted by stellar models. The possibility that these stars are of larger mass is briefly discussed." @default.
• W2108571343 created "2016-06-24" @default.
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• W2108571343 date "2010-05-05" @default.
• W2108571343 modified "2023-10-18" @default.
• W2108571343 title "FLUORINE ABUNDANCES IN GALACTIC ASYMPTOTIC GIANT BRANCH STARS" @default.
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• W2108571343 doi "https://doi.org/10.1088/2041-8205/715/2/l94" @default.
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