THE AGE AND DISTANCE OF THE KEPLER OPEN CLUSTER NGC 6811 FROM AN ECLIPSING BINARY, TURNOFF STAR PULSATION, AND GIANT ASTEROSEISMOLOGY

Research output: Research - peer-reviewJournal article

DOI

  • Eric L. Sandquist
    Eric L. SandquistSan Diego State Univ, California State University System, San Diego State University, Dept Astron
  • J. Jessen-Hansen
  • Matthew D. Shetrone
    Matthew D. ShetroneUniv Texas Austin, University of Texas Austin, McDonald Observ
  • Karsten Brogaard
  • Soren Meibom
    Soren MeibomHarvard Smithsonian Ctr Astrophys, Harvard University, Smithsonian Institution
  • Marika Leitner
    Marika LeitnerHumboldt State Univ, California State University System, Humboldt State University, Dept Phys & Astron
  • Dennis Stello
    Dennis StelloUniv Sydney, University of Sydney, Sydney Inst Astron SIfA, Sch Phys
  • Hans Bruntt
  • Victoria Antoci
  • Jerome A. Orosz
    Jerome A. OroszSan Diego State Univ, California State University System, San Diego State University, Dept Astron
  • Frank Grundahl
  • Søren Frandsen
Original languageEnglish
Article number11
JournalAstrophysical Journal Supplement Series
Volume831
Issue number1
Number of pages36
ISSN0004-637X
DOIs
StatePublished - 1 Nov 2016

    Research areas

  • asteroseismology, binaries: eclipsing, binaries: spectroscopic, open clusters and associations: individual (NGC 6811), stars: distances, stars: variables: delta Scuti, STELLAR POPULATION SYNTHESIS, ATMOSPHERIC VELOCITY-FIELDS, SOLAR CHEMICAL-COMPOSITION, HOBBY-EBERLY TELESCOPE, F-TYPE STARS, RED GIANTS, ABSOLUTE DIMENSIONS, MAIN-SEQUENCE, DELTA-SCUTI, AM STARS

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