Research ArticleASTROPHYSICS

Precise stellar surface gravities from the time scales of convectively driven brightness variations

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Science Advances  01 Jan 2016:
Vol. 2, no. 1, e1500654
DOI: 10.1126/sciadv.1500654

Article Information

vol. 2 no. 1

Online ISSN: 
History: 
  • Received for publication May 21, 2015
  • Accepted for publication November 4, 2015

Author Information

  1. Thomas Kallinger1,*,
  2. Saskia Hekker2,3,
  3. Rafael A. García4,
  4. Daniel Huber5,6,3 and
  5. Jaymie M. Matthews7
  1. 1Institute of Astrophysics, University of Vienna, Türkenschanzstrasse 17, Vienna 1180, Austria.
  2. 2Max-Planck-Institute für Sonnensystemforschung, Justus-von-Liebig-Weg 3, Göttingen 37077, Germany.
  3. 3Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, Aarhus C 8000, Denmark.
  4. 4Laboratoire AIM, CEA/DSM–CNRS, Université Paris Diderot–IRFU/SAp, Centre de Saclay, Gif-sur-Yvette Cedex 91191, France.
  5. 5Sydney Institute for Astronomy, School of Physics, University of Sydney, Sydney, New South Wales 2006, Australia.
  6. 6SETI Institute, 189 Bernardo Avenue, Mountain View, CA 94043, USA.
  7. 7Department of Physics and Astronomy, University of British Columbia, 6224 Agricultural Road, Vancouver, British Columbia V6T 1Z1, Canada.
  1. *Corresponding author. E-mail: thomas.kallinger{at}univie.ac.at

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