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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

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: A43. doi:10.1051/0004-6361/201525874.

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 Creators:
Beeck, B.1, Author           
Schüssler, M.2, 3, Author           
Cameron, R. H.4, 5, Author           
Reiners, A., Author
Affiliations:
1IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              
3Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
4Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              
5Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              

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 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: Theory: MHD Solar
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 Dates: 2015
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/201525874
BibTex Citekey: Beeck:2015-095
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 581 Sequence Number: A43 Start / End Page: - Identifier: -