Search Results for author: K. Lind

Found 2 papers, 1 papers with code

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3D NLTE spectral line formation of lithium in late-type stars

1 code implementation • 28 Oct 2020 • E. Wang, T. Nordlander, M. Asplund, A. M. Amarsi, K. Lind, Y. Zhou

Accurately known stellar lithium abundances may be used to shed light on a variety of astrophysical phenomena such as Big Bang nucleosynthesis, radial migration, ages of stars and stellar clusters, and planet engulfment events.

Solar and Stellar Astrophysics

2
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Effective temperature determinations of late-type stars based on 3D non-LTE Balmer line formation

no code implementations • 6 Apr 2018 • A. M. Amarsi, T. Nordlander, P. S. Barklem, M. Asplund, R. Collet, K. Lind

Hydrogen Balmer lines are commonly used as spectroscopic effective temperature diagnostics of late-type stars.

Solar and Stellar Astrophysics

 
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