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Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars

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Yadav,  Rakesh K.
IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Christensen,  Ulrich R.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Gastine,  Thomas
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Yadav, R. K., Christensen, U. R., Morin, J., Gastine, T., Reiners, A., Poppenhaeger, K., et al. (2015). Explaining the coexistence of large-scale and small-scale magnetic fields in fully convective stars. Astrophysical Journal, 813: L31. doi:10.1088/2041-8205/813/2/L31.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0029-B85F-2
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