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

Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaperJournal articleResearchpeer-review

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, Univ Sydney, University of Sydney, Sch Phys, Sydney Inst Astron
  • ,
  • 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
Issue2
Pages (from-to)2183–2195
ISSN0035-8711
DOIs
Publication statusPublished - 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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ID: 128526192