Stellar diameters and temperatures - VI. High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfs

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DOI

    Tabetha Boyajian, Yale School of Forestry and Environmental Studies, Kaspar von Braun, Max-Planck-Institut für Astronomie, Königstuhl 17, 69117, Heidelberg, Germany, Mirasol Institute, Lowell Observatory, Gregory A. Feiden, Uppsala universitet, Daniel Huber, NASA Ames Research Center, SETI Institute, Sarbani Basu, Yale School of Forestry and Environmental Studies, Pierre Demarque, Yale School of Forestry and Environmental Studies, Debra A. Fischer, Yale School of Forestry and Environmental Studies, Gail Schaefer, Mount Wilson Observatory, Andrew W. Mann, University of Texas, Austin, Texas,
  • Timothy R. White
  • Vicente Maestro, Sydney University, Sydney, John Brewer, Yale School of Forestry and Environmental Studies, C. Brooke Lamell, Yale School of Forestry and Environmental Studies, Federico Spada, Leibniz-Institut für Astrophysik Potsdam, Mercedes López-Morales, Harvard-Smithsonian Center for Astrophysics, Michael Ireland, RSSS, Australian National University, Chris Farrington, Mount Wilson Observatory, Gerard T. van Belle, Lowell Observatory, Stephen R. Kane, San Francisco State University, Jeremy Jones, Georgia State University, Theo A. ten Brummelaar, Mount Wilson Observatory, David R. Ciardi, California Institute of Technology, Harold A. McAlister, Georgia State University, Stephen Ridgway, National Optical Astronomy Observatory, P. J. Goldfinger, Mount Wilson Observatory, Nils H. Turner, Mount Wilson Observatory, Laszlo Sturmann, Mount Wilson Observatory
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume447
Issue number1
Pages (from-to)846-857
Number of pages12
ISSN0035-8711
DOIs
Publication statusPublished - 11 Feb 2015
Externally publishedYes

    Research areas

  • Infrared: stars, stars: fundamental parameters, Stars: individual: HD 189733, Stars: individual: HD 209458, Stars: late-type, Techniques: interferometric

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