Vv. Kovtyukh et Ni. Gorlova, Precise temperatures of classical Cepheids and yellow supergiants from line-depth ratios, ASTRON ASTR, 358(2), 2000, pp. 587-592
The ratios of spectral line-depths are powerful indicators of the effective
temperature. Thirty-two functional formulas to estimate the effective temp
eratures from line-depth ratios for Cepheids and F-G supergiants are offere
d. For high-quality spectra we find errors in the temperature as small as 1
0-15 K. These calibrations are only little sensitive to other stellar param
eters and allow to derive highly precise T-eff for supergiants in the range
4700-6700 K.