STELLAR DIAMETERS AND TEMPERATURES. III. MAIN-SEQUENCE A, F, G, AND K STARS: ADDITIONAL HIGH-PRECISION MEASUREMENTS AND EMPIRICAL RELATIONS

@article{Boyajian2013STELLARDA,
  title={STELLAR DIAMETERS AND TEMPERATURES. III. MAIN-SEQUENCE A, F, G, AND K STARS: ADDITIONAL HIGH-PRECISION MEASUREMENTS AND EMPIRICAL RELATIONS},
  author={Tabetha Boyajian and Kaspar von Braun and Gerard T. van Belle and Christopher D. Farrington and Gail H. Schaefer and Jeremy Jones and Russel J. White and Harold A. Mcalister and Theo A. ten Brummelaar and Stephen T. Ridgway and Douglas R. Gies and Laszlo Sturmann and Judit Sturmann and Nils H. Turner and P. J. Goldfinger and Norm Vargas},
  journal={The Astrophysical Journal},
  year={2013},
  volume={771},
  pages={40}
}
Based on CHARA Array measurements, we present the angular diameters of 23 nearby, main-sequence stars, ranging from spectral types A7 to K0, 5 of which are exoplanet host stars. We derive linear radii, effective temperatures, and absolute luminosities of the stars using Hipparcos parallaxes and measured bolometric fluxes. The new data are combined with previously published values to create an Angular Diameter Anthology of measured angular diameters to main-sequence stars (luminosity classes V… Expand
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