Figure 3 from Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars

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Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars

Authors: Tabetha S. Boyajian, Harold A. McAlister, Gerard van Belle, Douglas R. Gies, Theo A. ten Brummelaar, Kaspar von Braun, Chris Farrington, P. J. Goldfinger, David O'Brien, J. Robert Parks, Noel D. Richardson, Stephen Ridgway, Gail Schaefer, Laszlo Sturmann, Judit Sturmann, Yamina Touhami, Nils H. Turner, and Russel White

Boyajian et al. 2012 The Astrophysical Journal 746 101.

Provider: AAS Journals

Caption: Figure 3.

Top: the difference between limb-darkened angular diameters and the SED angular diameters from this work vs. ( B − V) color index. Bottom: the same as above with respect to metallicity. The dotted line shows an equal agreement of both measurements. A provisional fit to the data is shown as a solid line and is suspect to a cautious interpretation due to the sparse amount of data available. See Section 3 for details.

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