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Fig. 4
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Fundamental parameters of stars in empirical samples of Paper I. Left panel: log g vs. V0 - K0 compared to coefficients from Bessell et al. (1998) (see Table 1). Right panel: [Fe/H] vs. V0 - K0. The models used for the comparison of theoretical and empirical SBCRs have solar metallicities [Fe/H] = 0.
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