Comparing the Sun with other stars along the temperature coordinate

Physics

Scientific paper

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Line Spectra, Solar Temperature, Stellar Color, Stellar Temperature, Temperature Measurement, Metallicity, Stellar Physics

Scientific paper

The temperature of the Sun relative to other stars is determined using high-precision measurements of the ratios of depths of spectral lines. In effect, the Sun is placed within the stellar grid of relative temperatures with an estimated uncertainty of +/- 10 K. Among others, 16 Cyg A is found to be 5 +/- 12 K hotter than the Sun, while 16 Cyg B is found to be 45 +/- 12 K cooler than the Sun. In a similar manner, color indices are inferred with the results that R-I = 0.338 +/- 0.002 on the Cousins system and B-V = 0.648 +/- 0.006. This latter value supersedes the value of 0.656 published in 1992.

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