Table 4.
Data obtained from the isochrones to compute the ratio of subsamples A and B.
Metallicity | Mixture | V(TO) | Mini(TO) | V(TO) + 1 | Mini(V(TO) + 1) | V(TP-AGB) | Mini(TP-AGB) |
---|---|---|---|---|---|---|---|
−0.49 | 4.75 | 0.879 | 5.75 | 0.796 | −1.08 | 0.965 | |
−0.77 | 1P | 4.74 | 0.819 | 5.73 | 0.742 | −1.43 | 0.891 |
−1.29 | 4.51 | 0.773 | 5.51 | 0.704 | −1.86 | 0.830 | |
−1.60 | 4.42 | 0.756 | 5.41 | 0.694 | −1.93 | 0.800 | |
−0.49 | 4.83 | 0.822 | 5.82 | 0.744 | −1.13 | 0.899 | |
−0.77 | 4.86 | 0.753 | 5.85 | 0.683 | −1.47 | 0.819 | |
−1.29 | 2P | 4.59 | 0.708 | 5.59 | 0.646 | −1.86 | 0.756 |
−1.60 | 4.51 | 0.692 | 5.49 | 0.638 | −1.88 | 0.730 |
Notes. The reference metallicity and chemical mixtures are presented in the first two columns. From the third column on, we show the data obtained from the isochrones: absolute V magnitude in the turn-off [V(TO)] and its stellar mass [Mini(TO)]; absolute V magnitude of the nearest-neighbour star one magnitude fainter than the turn-off [V(TO) + 1] and its initial mass [Mini(V(TO) + 1)]; absolute V magnitude of a star at the beginning of the TP-AGB phase [V(TP-AGB)] and its initial mass [Mini(TP-AGB)].
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