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Published September 17, 2022 | Version v4
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Grid/NLTE

  • 1. Uppsala University

Description

Departure coefficients for iron in late-type stars.

See 3D non-LTE iron abundances in FG-type dwarfs (Amarsi, Liljegren, Nissen, A&A, in press) and Non-LTE departure coefficients for large spectroscopic surveys (Amarsi et al., A&A, 2020, 642, A62).

 

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atmos_Fe.txt

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