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 journal/Conference contribution in journal/Contribution to newspaperJournal articleResearchpeer-review

DOI

  • K. Brogaard
  • C. J. Hansen, Univ Copenhagen, Niels Bohr Institute, University of Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr,
  • A. Miglio
  • D. Slumstrup
  • S. Frandsen
  • J. Jessen-Hansen
  • M. N. Lund
  • D. Bossini, Univ Birmingham, University of Birmingham, Sch Phys & Astron, A. Thygesen, CALTECH, California Institute of Technology, G. R. Davies, Univ Birmingham, University of Birmingham, Sch Phys & Astron, W. J. Chaplin, Univ Birmingham, University of Birmingham, Sch Phys & Astron,
  • T. Arentoft
  • H. Bruntt,
  • F. Grundahl
  • R. Handberg
Original languageEnglish
JournalRoyal Astronomical Society. Monthly Notices
Volume476
Issue number3
Pages (from-to)3729-3743
Number of pages15
ISSN0035-8711
DOIs
Publication statusPublished - May 2018

    Research areas

  • binaries, eclipsing-stars, evolution-stars, fundamental parameters-stars, individual, MC 7037405, KIC 9540226, KIC 9970396-Galaxy, stellar content, SOLAR-LIKE OSCILLATIONS, OPEN CLUSTERS, LIGHT CURVES, KEPLER, BINARIES, MISSION, PARAMETERS, SPECTRA, CATALOG, AGES

See relations at Aarhus University Citationformats

ID: 127121731