Research ArticleASTRONOMY

Shape of a slowly rotating star measured by asteroseismology

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Science Advances  16 Nov 2016:
Vol. 2, no. 11, e1601777
DOI: 10.1126/sciadv.1601777

Article Information

vol. 2 no. 11

Online ISSN: 
History: 
  • Received for publication August 1, 2016
  • Accepted for publication October 12, 2016
  • .

Author Information

  1. Laurent Gizon1,2,3,4,*,
  2. Takashi Sekii3,
  3. Masao Takata5,
  4. Donald W. Kurtz6,
  5. Hiromoto Shibahashi5,
  6. Michael Bazot4,
  7. Othman Benomar4,5,
  8. Aaron C. Birch1 and
  9. Katepalli R. Sreenivasan4,7
  1. 1Max-Planck-Institut für Sonnensystemforschung, 37077 Göttingen, Germany.
  2. 2Institut für Astrophysik, Georg-August-Universität Göttingen, 37077 Göttingen, Germany.
  3. 3National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan.
  4. 4Center for Space Science, NYUAD Institute, New York University Abu Dhabi, P.O. Box 129188, Abu Dhabi, UAE.
  5. 5Department of Astronomy, The University of Tokyo, Bunkyo-ku, Tokyo 113-0033, Japan.
  6. 6Jeremiah Horrocks Institute, University of Central Lancashire, Preston PR1 2HE, UK.
  7. 7New York University, New York, NY 10012, USA.
  1. *Corresponding author. Email: gizon{at}mps.mpg.de

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