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Fig. A.2

image

Comparison of bolometric luminosities derived using different calibrations of MV with those derived for the same discrete MK spectral types and luminosity classes using integrated fluxes that are identified here with log L(λ1,D) /L (red lines). The identifications are dJM (de Jager & Nieuwenhuijzen 1987), DDS (Deutschman et al. 1976), SK (Aller et al. 1982), and W (Wegner 2006). The blocks a), b), and c) are for average MK luminosity classes V, IV, and III, respectively.

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