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- W2019203896 endingPage "566" @default.
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- W2019203896 abstract "Based on the analysis of high-resolution spectra with a high signal-to-noise ratio, we have determined the abundances of the α-elements O, Si, Ca and Ti, the iron peak elements V, Fe and Ni, and the heavy element Ba without the consideration of non-local thermodynamic equilibrium (NLTE) effect and the light neutron-rich elements Na, Mg and Al with an NLTE analysis for 63 nearby red clump giants. Fe abundances cover a logarithmic range between -0.60 and +0.35 relative to solar. All abundance ratios with respect to Fe are similar to those found in the Sun. Hyperfine structure (HFS) was taken into account when calculating V lines. The difference in abundances obtained with and without HFS can be as large as 0.5 dex." @default.
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- W2019203896 date "2007-11-07" @default.
- W2019203896 modified "2023-10-17" @default.
- W2019203896 title "The abundances of nearby red clump giants*" @default.
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- W2019203896 doi "https://doi.org/10.1111/j.1365-2966.2007.11852.x" @default.
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