Tag Archives: MARCS

NLTE line formation of Fe for late-type stars. I. Standard stars with 1D and model atmospheres

Maria Bergemann (1), K. Lind (1), R. Collet (2,3,1), Z. Magic (1) and M. Asplund (4,1) ((1)Max Planck Institute for Astrophysics, Karl-Schwarzschild Str. 1, 85741, Garching, Germany; (2) Natural History Museum of Denmark, Centre for Star and Planet Formation, Ă˜ster … Continue reading

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