Non-LTE line formation of Fe in late-type stars – IV. Modelling of the solar centre-to-limb variation in 3D
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DOI: 10.1093/mnras/stx673
Abstract: Our ability to model the shapes and strengths of iron lines in the solar spectrum is a critical test of the accuracy of the solar iron abundance, which sets the absolute zero-point of all stellar… read more here.
Keywords: non lte; line formation; lte line; formation late ... See more keywords