collaborators

1 paper

astro-ph.SR2017

Non-LTE line formation of Fe in late-type stars IV: Modelling of the solar centre-to-limb variation in 3D

K. Lind, A. M. Amarsi, M. Asplund +7

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…