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 for this work

Research output: Contribution to journal › Article › Academic › peer-review

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Physics