A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars

Dennis Stello (), Matteo Cantiello, Jim Fuller, Daniel Huber, Rafael A. García, Timothy R. Bedding, Lars Bildsten and Victor Silva Aguirre
Additional contact information
Dennis Stello: Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney
Matteo Cantiello: Kavli Institute for Theoretical Physics, University of California
Jim Fuller: Kavli Institute for Theoretical Physics, University of California
Daniel Huber: Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney
Rafael A. García: Laboratoire AIM, CEA/DSM—CNRS—Université Paris Diderot—IRFU/SAp Centre de Saclay
Timothy R. Bedding: Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney
Lars Bildsten: Kavli Institute for Theoretical Physics, University of California
Victor Silva Aguirre: Stellar Astrophysics Centre, Aarhus University

Nature, 2016, vol. 529, issue 7586, 364-367

Abstract: Suppression of dipolar oscillation modes by strong magnetic fields in the cores of intermediate-mass red giant stars reveals that powerful magnetic dynamos were very common in the previously convective cores of these stars.

Date: 2016
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DOI: 10.1038/nature16171

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