Table 1.
Main structural properties of our stellar models.
M/M⊙ | τH | τHe | τEAGB | τAGB | ![]() |
Mf/M⊙ | Lmax/L⊙ | ![]() |
(C/O)f |
---|---|---|---|---|---|---|---|---|---|
Z = 0.03 | |||||||||
1.00 | 1.14(10) | 8.65(7) | 2.76(7) | 7.57(5) | 0.538 | 0.560 | 4.86(3) | 2.24(6) | 0.38 |
1.25 | 4.91(9) | 1.12(8) | 1.73(7) | 1.14(6) | 0.539 | 0.582 | 6.30(3) | 2.98(6) | 0.38 |
1.50 | 2.77(9) | 1.09(8) | 2.90(7) | 1.16(6) | 0.551 | 0.615 | 8.17(3) | 3.68(6) | 0.34 |
2.00 | 1.20(9) | 1.51(8) | 1.93(7) | 2.34(6) | 0.530 | 0.653 | 1.12(4) | 6.73(6) | 1.03 |
2.50 | 6.35(8) | 2.11(8) | 2.16(7) | 2.61(6) | 0.527 | 0.688 | 1.45(4) | 1.35(7) | 1.08 |
3.00 | 3.83(8) | 1.11(8) | 1.20(7) | 1.71(6) | 0.575 | 0.699 | 1.56(4) | 2.15(7) | 1.27 |
3.50 | 2.52(8) | 6.38(7) | 6.41(6) | 9.77(5) | 0.662 | 0.786 | 2.20(4) | 5.45(7) | 1.09 |
4.00 | 1.76(8) | 3.92(7) | 3.73(6) | 4.12(5) | 0.766 | 0.849 | 2.89(4) | 7.55(7) | 0.018 |
4.50 | 1.30(8) | 2.67(7) | 2.22(6) | 2.35(5) | 0.837 | 0.893 | 3.72(4) | 8.09(7) | 0.075 |
5.00 | 9.94(7) | 1.89(7) | 1.53(6) | 2.02(5) | 0.869 | 0.922 | 4.37(4) | 8.28(7) | 0.065 |
5.50 | 7.89(7) | 1.45(7) | 1.01(6) | 1.65(5) | 0.905 | 0.951 | 5.13(4) | 8.51(7) | 0.031 |
6.00 | 6.42(7) | 1.09(7) | 7.38(5) | 1.35(5) | 0.940 | 0.972 | 6.10(4) | 8.75(7) | 0.032 |
6.50 | 5.36(7) | 8.74(6) | 5.11(5) | 1.01(5) | 0.990 | 1.022 | 7.06(4) | 9.06(7) | 0.030 |
7.00 | 4.53(7) | 7.59(6) | 3.11(5) | 8.39(4) | 1.095 | 1.052 | 8.04(4) | 9.38(7) | 0.033 |
8.00 | 3.42(7) | 5.34(6) | 1.99(5) | 4.32(4) | 0.000 | 1.210 | 9.57(4) | 9.91(7) | 0.048 |
Z = 0.04 | |||||||||
1.00 | 1.35(10) | 1.31(8) | 1.82(7) | 6.92(5) | 0.540 | 0.560 | 4.74(3) | 2.26(6) | 0.38 |
1.25 | 5.73(9) | 1.21(8) | 1.91(7) | 1.03(6) | 0.551 | 0.578 | 5.98(3) | 2.92(6) | 0.38 |
1.50 | 3.19(9) | 1.28(8) | 1.56(7) | 1.37(6) | 0.550 | 0.608 | 7.87(3) | 3.73(6) | 0.35 |
2.00 | 1.38(9) | 1.52(8) | 2.30(7) | 2.12(6) | 0.538 | 0.666 | 1.14(4) | 6.08(6) | 0.59 |
2.50 | 7.07(8) | 2.32(8) | 2.39(7) | 2.58(6) | 0.543 | 0.699 | 1.40(4) | 1.13(7) | 1.08 |
3.00 | 4.21(8) | 1.19(8) | 1.41(7) | 2.02(6) | 0.574 | 0.732 | 1.67(4) | 2.06(7) | 0.83 |
3.50 | 2.73(8) | 6.89(7) | 7.73(6) | 1.18(6) | 0.648 | 0.769 | 2.00(4) | 4.79(7) | 0.88 |
4.00 | 1.90(8) | 4.31(7) | 4.47(6) | 5.02(5) | 0.744 | 0.839 | 2.84(4) | 7.10(7) | 0.017 |
4.50 | 1.39(8) | 2.93(7) | 2.81(6) | 2.54(5) | 0.834 | 0.882 | 3.65(4) | 7.80(7) | 0.019 |
5.00 | 1.05(8) | 2.12(7) | 1.86(6) | 2.18(5) | 0.866 | 0.908 | 4.26(4) | 8.05(7) | 0.022 |
5.50 | 8.27(7) | 1.48(7) | 1.29(6) | 1.71(5) | 0.900 | 0.946 | 5.04(4) | 8.17(7) | 0.021 |
6.00 | 6.71(7) | 1.18(7) | 9.43(5) | 1.53(5) | 0.928 | 0.957 | 5.82(4) | 8.45(7) | 0.022 |
6.50 | 5.56(7) | 9.30(6) | 6.72(5) | 1.33(5) | 0.968 | 1.023 | 6.76(4) | 8.63(7) | 0.027 |
7.00 | 4.67(7) | 7.43(6) | 5.09(5) | 9.88(4) | 1.010 | 1.031 | 7.53(4) | 8.73(7) | 0.028 |
8.00 | 3.49(7) | 5.06(6) | 2.87(5) | 4.31(4) | 0.000 | 1.180 | 8.53(4) | 8.93(7) | 0.031 |
Notes. Columns are: initial mass in units of M⊙; duration of core H burning (τH), core He burning (τHe), early AGB (τEAGB) and thermally pulsating (τAGB) AGB phases; the core mass at the first TP ; the final mass of the star (Mf); the maximum luminosity (Lmax) and temperature at the bottom of the convective envelope (
) reached during the AGB phase; and the final C/O surface ratio. Timescales, luminosities, and temperatures are given as x(y), where x(y) = x × 10y.
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