Establishing the accuracy of asteroseismic mass and radius estimates of giant stars - I. Three eclipsing systems at [Fe/H] similar to-0.3 and the need for a large high-precision sample

Research output: Contribution to journalJournal articleResearchpeer-review

  • K. Brogaard
  • C. J. Hansen
  • A. Miglio
  • Ditte Slumstrup
  • S. Frandsen
  • J. Jessen-Hansen
  • M. N. Lund
  • D. Bossini
  • A. Thygesen
  • G. R. Davies
  • W. J. Chaplin
  • T. Arentoft
  • H. Bruntt
  • F. Grundahl
  • R. Handberg
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume476
Issue number3
Pages (from-to)3729-3743
ISSN0035-8711
DOIs
Publication statusPublished - 1 Feb 2018

    Research areas

  • binaries, eclipsing-stars, evolution-stars, fundamental parameters-stars, individual, MC 7037405, KIC 9540226, KIC 9970396-Galaxy, stellar content

Links

ID: 196374512