An astrophysical interpretation of the remarkable g-mode frequency groups of the rapidly rotating gamma Dor star, KIC 5608334

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DOI

    Hideyuki Saio, Tohoku Univ, Tohoku University, Grad Sch Sci, Astron Inst, Timothy R. Bedding, Univ Sydney, University of Sydney, Sch Phys, Sydney Inst Astron, Donald W. Kurtz, Univ Cent Lancashire, University of Central Lancashire, Jeremiah Horrocks Inst,
  • Simon J. Murphy
  • Victoria Antoci
  • Hiromoto Shibahashi, Univ Tokyo, University of Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Gang Li, Aarhus Univ, Aarhus University, Dept Phys & Astron, Stellar Astrophys Ctr, Masao Takata, Univ Tokyo, University of Tokyo, Sch Sci, Dept Astron, Bunkyo Ku
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume477
Issue number2
Pages (from-to)2183–2195
ISSN0035-8711
DOIs
StatePublished - Jun 2018

    Research areas

  • asteroseismology, stars: individual: (KIC 5608334), stars: oscillations, stars: rotation, stars: variables, TO-CORE ROTATION, ORDER G-MODES, MAIN-SEQUENCE, INTERNAL-ROTATION, DORADUS STARS, ASTEROSEISMIC MEASUREMENT, ANGULAR-DEPENDENCE, KEPLER DATA, OSCILLATIONS, SPB

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