Grid/NLTE
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Departure coefficients for iron in late-type stars. See <em>3D non-LTE iron abundances in FG-type dwarfs</em> (Amarsi, Liljegren, Nissen, A&A, in press) and <em>Non-LTE departure coefficients for large spectroscopic surveys</em> (Amarsi et al., A&A, 2020, 642, A62).
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Zenodo创建时间：
2022-09-26
