Physics
Scientific paper
Feb 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995pasp..107..120g&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 107, no. 708, p. 120-123
Physics
29
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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