Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...301..868s&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 301, Feb. 15, 1986, p. 868-876.
Astronomy and Astrophysics
Astrophysics
7
K Stars, Red Giant Stars, Stellar Atmospheres, Stellar Color, Stellar Models, Stellar Spectrophotometry, Stellar Temperature, Limb Darkening, M Stars, Molecular Spectra
Scientific paper
Photometric parameters in the Johnson broad-band and Wing narrow-band photometric systems have been computed for 24 stellar atmospheric models of K and M giants of Johnson, Bernat, and Krupp (1980). Color temperatures, color indices, and certain molecular indices predicted by these models are compared with observations of M giant stars. Good agreement is obtained for effective temperatures of 3500 K or greater, which provides evidence for the overall accuracy of the models. The comparisons support the higher effective temperature scales of Tsuji (1978, 1981) and Ridgway et al. (1980). For models with effective temperatures below 3500 K, the TiO bands are systematically too weak relative to observations. Possible reasons for this discrepancy are discussed. The comparison of broadband color indices gives information concerning the surface gravities. The effects of limb darkening and possible variation of photospheric radius with wavelength on predicted broad-band model colors, and additional implications of comparison between theory and observations, are discussed.
Johnson Hollis R.
Steiman-Cameron Thomas Y.
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