Non-LTE line formation of Fe in late-type stars - I. Standard stars with 1D and 〈3D〉 model atmospheres

Maria Bergemann*, K. Lind, R. Collet, Z. Magic, M. Asplund

*Corresponding author for this work

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

    281 Citations (SciVal)

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    Physics