Absolute Magnitudes of Seismic Red Clumps in the Kepler Field and SAGA: The Age Dependency of the Distance Scale

Research output: Research - peer-reviewJournal article

DOI

  • Y. Q. Chen
    Y. Q. ChenNatl Opt Astron ObservChinese Acad Sci, Chinese Academy of Sciences, Natl Astron Observ, Key Lab Opt AstronChinese Acad Sci, Chinese Academy of Sciences, Guangxi Inst BotChinese Academy of SciencesUniv Chinese Acad Sci, Chinese Academy of Sciences, University of Chinese Academy of Sciences, Sino Danish Ctr Educ & ResUniversity of the Chinese Academy of SciencesSt Marys Univ, Saint Marys University - Canada, Dept Phys & Astron, Inst Computat AstrophysUniv Toronto, University of Toronto, CITAUniversity of Toronto, St. Michael's Hospital, Toronto
  • L. Casagrande
    L. CasagrandeRSPAS, Australian National University
  • G. Zhao
    G. ZhaoUniversity of the Chinese Academy of Sciences
  • Jo Bovy
    Jo BovyUniversity of Toronto, St. Michael's Hospital, Toronto
  • V. Silva Aguirre
  • J. K. Zhao
    J. K. ZhaoNatl Opt Astron ObservChinese Acad Sci, Chinese Academy of Sciences, Natl Astron Observ, Key Lab Opt AstronChinese Acad Sci, Chinese Academy of Sciences, Guangxi Inst BotChinese Academy of Sciences
  • Y. P. Jia
    Y. P. JiaUniversity of the Chinese Academy of Sciences
Original languageEnglish
Article number77
JournalAstrophysical Journal
Volume840
Issue number2
Number of pages11
ISSN0004-637X
DOIs
StatePublished - 10 May 2017

    Research areas

  • asteroseismology, stars: fundamental parameters, stars: distances, stars: late-type, surveys, K-BAND MAGNITUDE, GIANT STARS, GALACTIC ARCHAEOLOGY, STELLAR POPULATIONS, ECLIPSING BINARIES, INPUT CATALOG, CHARA ARRAY, ASTEROSEISMOLOGY, CALIBRATION, CLUSTERS

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ID: 114838141