Oscillating red giants in eclipsing binary systems: empirical reference value for asteroseismic scaling relation

  • N Themeßl
    Max Planck Institute for Solar system Research, Justus-von-Liebig-Weg 3, D-37077 Göttingen, Germany
  • S Hekker
    Max Planck Institute for Solar system Research, Justus-von-Liebig-Weg 3, D-37077 Göttingen, Germany
  • J Southworth
    Astrophysics Group, Keele University, Staffordshire ST5 5BG, UK
  • P G Beck
    Instituto de Astrofísica de Canarias, E-38200 La Laguna, Tenerife, Spain
  • K Pavlovski
    Department of Physics, University of Zagreb, Bijenička Cesta 32, 10000 Zagreb, Croatia
  • A Tkachenko
    Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, B-3001 Leuven, Belgium
  • G C Angelou
    Max-Planck Institut für Astrophysik, Karl-Schwarzschild-Str 1, D-85741 Garching, Germany
  • W H Ball
    School of Physics and Astronomy, U. Birmingham, Edgbaston, Birmingham B15 2TT, UK
  • C Barban
    LESIA, PSL Research University, CNRS, Univ. Pierre et Marie Curie, Univ. Denis Diderot, Observatoire de Paris, F-92195 Meudon Cedex, France
  • E Corsaro
    INAF – Osservatorio Astrofisico di Catania, Via S. Sofia 78, I-95123 Catania, Italy
  • Y Elsworth
    School of Physics and Astronomy, U. Birmingham, Edgbaston, Birmingham B15 2TT, UK
  • R Handberg
    Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark
  • T Kallinger
    Institute for Astrophysics, University of Vienna, Türkenschanzstraße 17, A-1180 Vienna, Austria

書誌事項

公開日
2018-05-01
権利情報
  • http://academic.oup.com/journals/pages/about_us/legal/notices
DOI
  • 10.1093/mnras/sty1113
公開者
Oxford University Press (OUP)

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