Three-dimensional simulations of near-surface convection in main-sequence stars 
- IV. Effect of small-scale magnetic flux concentrations on centre-to-limb 
variation and spectral lines

Beeck, B.; Schüssler, M.; Cameron, R. H.; Reiners, A.

doi:10.1051/0004-6361/201525874

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Three-dimensional simulations of near-surface convection in main-sequence stars - IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral lines

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Beeck, B.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;

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Schüssler, M.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

/persons/resource/persons103859

Cameron, R. H.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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Beeck, B., Schüssler, M., Cameron, R. H., & Reiners, A. (2015). Three-dimensional simulations of near-surface convection in main-sequence stars - IV. Effect of small-scale magnetic flux concentrations on centre-to-limb variation and spectral lines. Astronomy and Astrophysics, 581:. doi:10.1051/0004-6361/201525874.

引用: https://hdl.handle.net/11858/00-001M-0000-0028-FF04-7

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