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MESA meets MURaM. Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations

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Ball,  W. H.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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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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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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Gizon,  L.
Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society;

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Ball, W. H., Beeck, B., Cameron, R. H., & Gizon, L. (2016). MESA meets MURaM. Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations. Astronomy and Astrophysics, 592: A159. doi:10.1051/0004-6361/201628300.


Cite as: https://hdl.handle.net/11858/00-001M-0000-002B-5FE6-5
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