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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作者：
Beeck, B. [1 ]
Schüssler, M. [1 ]
Cameron, R.H. [1 ]
Reiners, A. [2 ]
机构：
[1] Max-Planck-Institut für Sonnensystemforschung, Justus-von-Liebig-Weg 3, Göttingen,37077, Germany
[2] Institut für Astrophysik, Universität Göttingen, Friedrich-Hund-Platz 1, Göttingen,37077, Germany
来源：
Astronomy and Astrophysics | 2015年 / 581卷
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All Open Access; Bronze;
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摘要：
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