作者: T. V. Mishenina , V. V. Kovtyukh , S. A. Korotin , C. Soubiran
DOI: 10.1134/1.1575856
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摘要: The non-LTE sodium abundances of 100 stars with metallicities −3 3.8) −2<[Fe/H]<−1. observed relation between [Na/Fe] and [Fe/H] is in satisfactory agreement the theoretical computations Samland, which take into account metallicity dependence yield a number other factors affecting distribution elements Galaxy during course its evolution.