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Effective Temperatures and Angular Diameters of A–G Main Sequence Stars
Published online by Cambridge University Press: 12 April 2016
Abstract
For 9 stars of A5–G2 spectral type interval IV and V luminosity classes effective temperatures, bolometric corrections, radii, angular diameters and luminosities were obtained by means of the infrared flux method in the modification by Blackwell et al. (1980).
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- II. Atmospheres, a window to the interior
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- Copyright © Astronomical Society of the Pacific 1993