Abstract
The non-LTE sodium abundance has been determined from the Na I 6154 and 6161 Å lines for 38 thin-disk stars (15 of them are Ba II stars), 15 thick-disk stars, 13 Hercules-stream stars, and 13 stars that cannot be attributed neither to the thick Galactic disk nor to the thin one. The Na I model atom has been constructed using the most accurate present-day atomic data. For the Na I 6154 and 6161 Å lines, the non-LTEabundance corrections are from −0.06 to −0.24 dex, depending on the stellar parameters. No differences in [Na/Fe] abundance between the thick and thin disks have been detected; the derived ratios are close to the solar ones. The existence of a [Na/Fe] overabundance in the Ba II stars has been confirmed. The Hercules-stream stars exhibit nearly solar [Na/Fe] ratios. The results obtained can be used to test the sodium nucleosynthesis models.
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Original Russian Text © S.A. Alexeeva, Yu.V. Pakhomov, L.I. Mashonkina, 2014, published in Pis’ma v Astronomicheskiĭ Zhurnal, 2014, Vol. 40, No. 7, pp. 454–472.
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Alexeeva, S.A., Pakhomov, Y.V. & Mashonkina, L.I. Non-LTE sodium abundance in galactic thick- and thin-disk red giants. Astron. Lett. 40, 406–424 (2014). https://doi.org/10.1134/S1063773714070019
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DOI: https://doi.org/10.1134/S1063773714070019