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

Author

Listed:
  • Dennis Stello

    (Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney
    Stellar Astrophysics Centre, Aarhus University)

  • Matteo Cantiello

    (Kavli Institute for Theoretical Physics, University of California)

  • Jim Fuller

    (Kavli Institute for Theoretical Physics, University of California
    TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17, California Institute of Technology)

  • Daniel Huber

    (Sydney Institute for Astronomy (SIfA), School of Physics, University of Sydney
    Stellar Astrophysics Centre, Aarhus University
    SETI Institute)

  • 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
    Stellar Astrophysics Centre, Aarhus University)

  • Lars Bildsten

    (Kavli Institute for Theoretical Physics, University of California
    University of California)

  • Victor Silva Aguirre

    (Stellar Astrophysics Centre, Aarhus University)

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.

Suggested Citation

  • Dennis Stello & Matteo Cantiello & Jim Fuller & Daniel Huber & Rafael A. García & Timothy R. Bedding & Lars Bildsten & Victor Silva Aguirre, 2016. "A prevalence of dynamo-generated magnetic fields in the cores of intermediate-mass stars," Nature, Nature, vol. 529(7586), pages 364-367, January.
    • Handle: RePEc:nat:nature:v:529:y:2016:i:7586:d:10.1038_nature16171
    DOI: 10.1038/nature16171
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