Fig. 14

Atlas of spectra in the 6485–6510 Å region, containing the “quintet” of strong Ca I, Fe I, and Ba II lines. These and other prominent lines are indicated near the bottom axis. Normalized, telluric-line corrected spectra for MS stars are shown in black, in a temperature sequence (hotter to the bottom), and offset by 0.5 units for clarity. Red spectra are for giant stars at similar temperatures as the respective MS spectra. Gravity-sensitive lines stand out clearly from the comparison. Spectral ranges used to compute the βt index are indicated with cyan color (and the enclosed yellow range), while green ranges indicate the index reference continuum. Yellow ranges are instead used to compute the βc index, with the same reference continuum as for βt.
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