Oscillation mode linewidths and heights of 23 main-sequence stars observed by Kepler (Corrigendum)

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

    T. Appourchaux, Univ Paris 11, Centre National de la Recherche Scientifique (CNRS), University of Paris Sud - Paris XI, Universite Paris Saclay (ComUE), Inst Astrophys Spatiale, UMR 8617, CNRS, H. M. Antia, Tata Inst Fundamental Res, Tata Institute of Fundamental Research, O. Benomar, Univ Sydney, University of Sydney, Sch Phys, SIfA, Univ Tokyo, University of Tokyo, Dept Astron, T. L. Campante, Univ Birmingham, University of Birmingham, Sch Phys & Astron, G. R. Davies, Univ Birmingham, University of Birmingham, Sch Phys & Astron, Univ Paris Diderot, CEA, University of Paris Diderot - Paris VII, Universite Sorbonne Paris Cite-USPC (COMUE), Centre National de la Recherche Scientifique (CNRS), CEA DSM CNRS, Lab AIM, IRFU SAp,Ctr Saclay,
  • R. Handberg
  • R. Howe, Univ Birmingham, University of Birmingham, Sch Phys & Astron, C. Regulo, Instituto de Astrofísica de Canarias, Univ La Laguna, Universidad de la Laguna, Dept Astrofis, K. Belkacem, Univ Paris 07, Observatoire de Paris, University of Paris Diderot - Paris VII, Universite Sorbonne Paris Cite-USPC (COMUE), Pierre & Marie Curie University - Paris 6, PSL Research University Paris, UPMC, CNRS UMR 8109, LESIA,Observ Paris,
  • G. Houdek
  • R. A. Garcia, Univ Paris Diderot, CEA, University of Paris Diderot - Paris VII, Universite Sorbonne Paris Cite-USPC (COMUE), Centre National de la Recherche Scientifique (CNRS), CEA DSM CNRS, Lab AIM, IRFU SAp,Ctr Saclay, W. J. Chaplin, Univ Birmingham, University of Birmingham, Sch Phys & Astron
Original languageEnglish
Article number2
JournalAstronomy & Astrophysics
Volume595
Number of pages3
ISSN0004-6361
DOIs
StatePublished - 2016

    Research areas

  • stars: interiors, asteroseismology, methods: data analysis, errata, addenda

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