Asteroseismic Properties of Solar-type Stars Observed with the NASA K2 Mission: Results from Campaigns 1-3 and Prospects for Future Observations

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  • Mikkel N. Lund
  • William J. Chaplin, Univ Birmingham, University of Birmingham, Sch Phys & Astron, Aarhus Univ, Aarhus University, Stellar Astrophys Ctr, Dept Phys & Astron, Luca Casagrande, Australian Natl Univ, Australian National University, Res Sch Astron & Astrophys, Mt Stromlo Observ,
  • Victor Silva Aguirre
  • Sarbani Basu, Yale Univ, Yale University, Dept Astron, Allyson Bieryla, Harvard Smithsonian Ctr Astrophys, Harvard University, Smithsonian Institution,
  • Jorgen Christensen-Dalsgaard
  • David W. Latham, Harvard Smithsonian Ctr Astrophys, Harvard University, Smithsonian Institution,
  • Tim White
  • Guy R. Davies, Univ Birmingham, University of Birmingham, Sch Phys & Astron, Aarhus Univ, Aarhus University, Stellar Astrophys Ctr, Dept Phys & Astron, Daniel Huber, Aarhus Univ, Aarhus University, Stellar Astrophys Ctr, Dept Phys & Astron, Univ Sydney, University of Sydney, SIfA, Sch Phys, SETI Inst, Lars A. Buchhave, Univ Copenhagen, University of Copenhagen, Ctr Star & Planet Format, Nat Hist Museum Denmark, Univ Copenhagen, Niels Bohr Institute, University of Copenhagen, Niels Bohr Inst,
  • Rasmus Handberg
Original languageEnglish
Article number124204
JournalPublications of the Astrnomical Society of the Pacific (PASP)
Volume128
Issue number970
Number of pages19
ISSN0004-6280
DOIs
StatePublished - Dec 2016

    Research areas

  • asteroseismology, methods: data analysis, stars: distances, stars: fundamental parameters, stars: oscillations, stars: solar-type, GENEVA-COPENHAGEN SURVEY, STELLAR EVOLUTION CODE, SURFACE BRIGHTNESS RELATIONS, MASS-LUMINOSITY-RELATION, SPIN-ORBIT MISALIGNMENT, MAIN-SEQUENCE STARS, FUNDAMENTAL PROPERTIES, GALACTIC ARCHAEOLOGY, KEPLER MISSION, OB ASSOCIATION

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ID: 108083750