Table 2.
Main characteristics of the TP-(S)AGB of our models.
Mini | NTP | τTP-(S)AGB | ΔtIP | Mc, ini | Mc, f | Menv, f | ⟨THeBS⟩ | ⟨THBS⟩ | ⟨TBCE⟩ |
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⟨λ⟩ | ⟨Ṁwind⟩ |
---|---|---|---|---|---|---|---|---|---|---|---|---|
(M⊙) | (Myr) | (yr) | (M⊙) | (M⊙) | (M⊙) | (MK) | (MK) | (MK) | (M⊙) | (M⊙ yr−1) | ||
Z = 10−10 | ||||||||||||
3★ | 35(2) | 0.78 | 17990 | 0.77 | 0.79 | < 0.1 | 313 | 82 | 36 | 0.14 | 0.87 | 2.8 × 10−6 |
4★ | 41(1) | 0.33 | 7712 | 0.85 | 0.87 | < 0.1 | 312 | 99 | 58 | 0.12 | 0.76 | 9.5 × 10−6 |
5♣ | 482 | 0.59 | 1471 | 0.89 | 1.14 | 3.08 | 223 | 157 | 26 | – | – | 1.3 × 10−6 |
6 | 77 | 0.99 | 2927 | 0.95 | 0.97 | < 0.1 | 331 | 111 | 86 | 0.19 | 0.80 | 2.9 × 10−5 |
7 | 69 | 0.13 | 1658 | 1.00 | 1.02 | < 0.1 | 329 | 116 | 103 | 0.05 | 0.71 | 4.7 × 10−5 |
7.5 | 82 | 0.09 | 1053 | 1.04 | 1.06 | 0.18 | 327 | 123 | 118 | 0.04 | 0.70 | 6.6 × 10−5 |
8.0 | 103 | 0.05 | 488 | 1.11 | 1.12 | 0.10 | 323 | 135 | 130 | 0.02 | 0.62 | 1.3 × 10−4 |
8.5 | 102 | 0.03 | 285 | 1.16 | 1.17 | 0.21 | 328 | 136 | 132 | 0.01 | 0.57 | 2.3 × 10−4 |
Z = 10−8 | ||||||||||||
3★ | 27(2) | 0.34 | 15206 | 0.81 | 0.83 | < 0.1 | 316 | 85 | 47 | 0.11 | 0.87 | 6.1 × 10−6 |
4★ | 36(1) | 0.30 | 6719 | 0.87 | 0.88 | < 0.1 | 318 | 104 | 61 | 0.11 | 0.77 | 1.0 × 10−5 |
5♣ | 402 | 0.54 | 1418 | 0.91 | 1.14 | 3.11 | 230 | 154 | 24 | – | – | 1.8 × 10−6 |
6 | 58 | 0.17 | 2693 | 0.96 | 0.97 | 0.12 | 322 | 114 | 81 | 0.29 | 0.70 | 2.9 × 10−5 |
7 | 69 | 0.11 | 1442 | 1.02 | 1.03 | < 0.1 | 323 | 120 | 107 | 0.07 | 0.57 | 5.3 × 10−5 |
7.5 | 82 | 0.10 | 983 | 1.06 | 1.07 | 0.17 | 329 | 123 | 118 | 0.03 | 0.70 | 6.4 × 10−5 |
8.0 | 95 | 0.05 | 492 | 1.12 | 1.13 | 0.18 | 330 | 138 | 133 | 0.02 | 0.63 | 1.3 × 10−4 |
8.5 | 97 | 0.04 | 296 | 1.17 | 1.18 | 0.23 | 331 | 134 | 130 | 0.01 | 0.60 | 2.0 × 10−4 |
Z = 10−7 | ||||||||||||
3★ | 24 | 0.38 | 12700 | 0.82 | 0.84 | < 0.1 | 310 | 94 | 46 | 0.10 | 0.75 | 5.6 × 10−6 |
4 | 38 | 0.28 | 78590 | 0.87 | 0.88 | < 0.1 | 317 | 105 | 58 | 0.19 | 0.69 | 1.1 × 10−5 |
5 | 60 | 0.07 | 3929 | 0.91 | 0.94 | < 0.1 | 311 | 109 | 76 | 0.06 | 0.57 | 1.6 × 10−5 |
6 | 58 | 0.05 | 2688 | 0.97 | 0.98 | < 0.1 | 327 | 114 | 86 | 0.06 | 0.73 | 1.1 × 10−5 |
7 | 72 | 0.01 | 1082 | 1.05 | 1.07 | < 0.1 | 326 | 122 | 116 | 0.04 | 0.70 | 5.6 × 10−5 |
7.5 | 85 | 0.06 | 534 | 1.11 | 1.12 | 0.09 | 324 | 131 | 126 | 0.05 | 0.64 | 1.0 × 10−4 |
8.0 | 72 | 0.02 | 285 | 1.18 | 1.19 | 0.25 | 336 | 130 | 125 | 0.007 | 0.61 | 3.2 × 10−4 |
8.5 | 87 | 0.002 | 153 | 1.23 | 1.24 | 0.24 | 347 | 131 | 126 | 0.009 | 0.50 | 4.5 × 10−4 |
Z = 10−6 | ||||||||||||
3 | 26 | 0.42 | 14140 | 0.82 | 0.84 | < 0.1 | 317 | 89 | 42 | 0.08 | 0.80 | 2.3 × 10−6 |
4 | 36 | 0.30 | 8424 | 0.87 | 0.88 | 0.22 | 325 | 96 | 65 | 0.15 | 0.86 | 9.7 × 10−6 |
5 | 45 | 0.27 | 5070 | 0.89 | 0.92 | < 0.1 | 326 | 104 | 75 | 0.06 | 0.82 | 1.5 × 10−5 |
6 | 54 | 0.13 | 2128 | 0.99 | 1.01 | 0.16 | 327 | 114 | 93 | 0.05 | 0.77 | 3.7 × 10−5 |
7 | 65 | 0.06 | 668 | 1.11 | 1.12 | 0.27 | 350 | 127 | 121 | 0.02 | 0.81 | 9.4 × 10−5 |
7.5 | 75 | 0.02 | 260 | 1.17 | 1.18 | 0.27 | 353 | 132 | 129 | 0.006 | 0.47 | 2.7 × 10−4 |
8.0 | 92 | 0.01 | 139 | 1.24 | 1.25 | 0.34 | 349 | 131 | 125 | 0.005 | 0.47 | 4.0 × 10−4 |
Notes. Models marked with a star (★) experience proton-ingestion episodes. Thermal pulses gradually decrease in intensity and vanish in the models marked with a club symbol (♣). In these cases models fail to converge while their convective envelopes have very high masses (≳3 M⊙), and thus their fates are unknown (see text for details). Mini corresponds to the initial mass. NTP is the number of thermal pulses and, in parenthesis, the number of proton-ingestion episodes. τTP-(S)AGB, and ΔtIP are, respectively, the duration of the TP-(S)AGB (given from the first thermal pulse until the end of our computations), and the interpulse period. Mc, ini, Mc, f and Menv, f are the masses of the H-exhausted cores prior to the TP-(S)AGB, the masses of the H-exhausted cores, and the remnant envelopes at the end of the TP-(S)AGB. ⟨THeBS⟩, ⟨THBS⟩, ⟨TBCE⟩ are the temperatures at the times of maximum luminosity for each pulse, given at the centre of the He-burning shell, at the centre of the H-burning shell, and at the base of the convective envelope, and averaged over the number of thermal pulses in each sequence. is the total mass dredged-up ⟨λ⟩ is averaged over the number of thermal pulses in each case, and ⟨Ṁwind⟩ is the average mass-loss rates due to winds, that is, the envelope mass lost over the duration of the (S)AGB phase.
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