STELLAR DIAMETERS AND TEMPERATURES. I. MAIN-SEQUENCE A, F, AND G STARS

@article{Boyajian2012STELLARDA,
  title={STELLAR DIAMETERS AND TEMPERATURES. I. MAIN-SEQUENCE A, F, AND G STARS},
  author={Tabetha S. Boyajian and Harold A. Mcalister and Gerard T. van Belle and Douglas R. Gies and Theo A. ten Brummelaar and Kaspar von Braun and Christopher D. Farrington and P. J. Goldfinger and David P. O'Brien and J. Robert Parks and Noel D. Richardson and Stephen T. Ridgway and Gail H. Schaefer and Laszlo Sturmann and Judit Sturmann and Yamina Touhami and Nils H. Turner and Russel J. White},
  journal={The Astrophysical Journal},
  year={2012},
  volume={746}
}
We have executed a survey of nearby, main-sequence A-, F-, and G-type stars with the CHARA Array, successfully measuring the angular diameters of forty-four stars with an average precision of ∼1.5%. We present new measures of the bolometric flux, which in turn leads to an empirical determination of the effective temperature for the stars observed. In addition, these CHARA-determined temperatures, radii, and luminosities are fit to Yonsei–Yale model isochrones to constrain the masses and ages of… 
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