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Asteroseismology can reveal strong internal magnetic fields in red giant stars

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Science  23 Oct 2015:
Vol. 350, Issue 6259, pp. 423-426
DOI: 10.1126/science.aac6933

Article Information

vol. 350 no. 6259 423-426

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History: 
  • Received for publication May 29, 2015
  • Accepted for publication September 15, 2015
  • .

Author Information

  1. Jim Fuller1,2,*,,
  2. Matteo Cantiello2,*,,
  3. Dennis Stello3,4,
  4. Rafael A. Garcia5,
  5. Lars Bildsten2,6
  1. 1TAPIR, Walter Burke Institute for Theoretical Physics, Mailcode 350-17 California Institute of Technology, Pasadena, CA 91125, USA.
  2. 2Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106, USA.
  3. 3Sydney Institute for Astronomy, School of Physics, University of Sydney, New South Wales 2006, Australia.
  4. 4Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark.
  5. 5Laboratoire Astrophysique Interactions Multi-échelles, Commissariat á l’Énergie Atomique/Direction des Sciences de la Matiére, CNRS, Université Paris Diderot, Institut de Recherches sur les lois Fondamentales de l’Univers/Service d’Astrophysique Centre de Saclay, 91191 Gif-sur-Yvette Cedex, France.
  6. 6Department of Physics, University of California, Santa Barbara, CA 93106, USA.
  1. *Corresponding author. E-mail: jfuller{at}caltech.edu (J.F.); matteo{at}kitp.ucsb.edu (M.C.)
  1. These authors contributed equally to this work.

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