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- W2121856211 abstract "Abundance analysis of the cool extreme helium (EHe) star LSS 3378 is presented. The abundance analysis is done using local thermodynamic equilibrium (LTE) line formation and LTE model atmospheres constructed for EHe stars.The atmosphere of LSS 3378 shows evidence of H-burning, He-burning, and s-process nucleosynthesis. The derived abundances of iron peak and α-elements indicate the absence of selective fractionation or any other processes that can distort chemical composition of these elements. Hence, the Fe abundance [log e(Fe) = 6.1] is adopted as an initial metallicity indicator. The measured abundances of LSS 3378 are compared with those of R Coronae Borealis (RCB) stars and with rest of the EHe stars as a group." @default.
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- W2121856211 date "2006-06-07" @default.
- W2121856211 modified "2023-09-23" @default.
- W2121856211 title "Abundance analysis of the cool extreme helium star LSS 3378" @default.
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- W2121856211 doi "https://doi.org/10.1111/j.1365-2966.2006.10398.x" @default.
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