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

Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaperJournal article

DOI

    Y. Q. Chen, Natl Opt Astron Observ, Chinese Acad Sci, Chinese Academy of Sciences, Natl Astron Observ, Key Lab Opt Astron, Chinese Acad Sci, Chinese Academy of Sciences, Guangxi Inst Bot, Chinese Academy of Sciences, Univ Chinese Acad Sci, Chinese Academy of Sciences, University of Chinese Academy of Sciences, Sino Danish Ctr Educ & Res, University of the Chinese Academy of Sciences, St Marys Univ, Saint Marys University - Canada, Dept Phys & Astron, Inst Computat Astrophys, Univ Toronto, University of Toronto, CITA, University of Toronto, St. Michael's Hospital, Toronto, L. Casagrande, RSPAS, Australian National University, G. Zhao, University of the Chinese Academy of Sciences, Jo Bovy, University of Toronto, St. Michael's Hospital, Toronto,
  • V. Silva Aguirre
  • J. K. Zhao, Natl Opt Astron Observ, Chinese Acad Sci, Chinese Academy of Sciences, Natl Astron Observ, Key Lab Opt Astron, Chinese Acad Sci, Chinese Academy of Sciences, Guangxi Inst Bot, Chinese Academy of Sciences, Y. P. Jia, University 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