Non-LTE abundance corrections for late-type stars from 2000 A to 3 μm: I. Na, Mg, and Al

K. Lind^*, T. Nordlander, A. Wehrhahn, M. Montelius, Y. Osorio, P. S. Barklem, M. Afşar, C. Sneden, C. Kobayashi

^*Corresponding author voor dit werk

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Non-LTE abundances for Na, Mg and Al
Lind, K. (Contributor), Nordlander, T. (Contributor), Wehrhahn, A. (Contributor), Schmidt Montelius, M. (Contributor), Osorio, Y. (Contributor), Barklem, P. S. (Contributor), Afşar, M. (Contributor), Sneden, C. (Contributor) & Kobayashi, C. (Contributor), Strasbourg Astronomical Data Center, 8-sep.-2022
DOI: 10.26093/cds/vizier.36650033
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