Table B.1
Main properties of the M15 sequences from the ZAMS to the TP-AGB.
| Mi | τMS | τRGB | HeCF | τHeCB | τeAGB |
|
τTP−AGB(M) | τTP−AGB(C) | #TP | Mf | NC/NO |
| [M⊙] | [Myr] | [Myr] | [Myr] | [Myr] | [M⊙] | [Myr] | [Myr] | (AGB) | [M⊙] | ||
|
|
|||||||||||
| Z0 = 0.01 | |||||||||||
|
|
|||||||||||
| 1.00 | 8539.1 | 1847.8 | yes | 112.45 | 10.825 | 0.5119 | 0.71950 | 0.0000 | 4 | 0.5282 | .404 |
| 1.50 | 1989.7 | 481.76 | yes | 102.81 | 9.6305 | 0.5271 | 0.81428 | 0.26368 | 7 | 0.5595 | 1.77 |
| 2.00 | 969.87 | 59.771 | no | 162.42 | 13.899 | 0.5062 | 1.5132 | 0.65170 | 12 | 0.5584 | 2.52 |
| 2.50 | 534.59 | 9.2022 | no | 165.72 | 10.055 | 0.5434 | 0.61113 | 1.1034 | 11 | 0.5678 | 3.80 |
| 3.00 | 334.09 | 4.2506 | no | 87.321 | 4.8755 | 0.6386 | 0.17697 | 0.34383 | 8 | 0.6352 | 3.16 |
| 4.00 | 164.01 | 1.4422 | no | 27.686 | 1.6394 | 0.8018 | 0.29503E-01 | 0.10702 | 11 | 0.7968 | 1.95 |
|
|
|||||||||||
| Z0 = 0.001 | |||||||||||
|
|
|||||||||||
| 1.00 | 5649.1 | 848.89 | yes | 86.936 | 8.5632 | 0.5240 | 0.62546 | 0.24255 | 4 | 0.5451 | 8.44 |
| 1.50 | 1342.9 | 319.05 | yes | 84.146 | 7.3278 | 0.5564 | 0.52748E-03 | 1.0151 | 7 | 0.5804 | 7.78 |
| 2.00 | 616.85 | 15.556 | no | 158.36 | 5.6971 | 0.6167 | 0.82512E-01 | 0.77219 | 10 | 0.6202 | 8.29 |
| 2.50 | 399.46 | 6.0777 | no | 82.517 | 3.3881 | 0.7021 | 0.20568E-03 | 0.56845 | 12 | 0.6916 | 7.03 |
Notes. Mi: initial mass of the model (at ZAMS). τMS: duration of the main sequence, until 
. τRGB: lifetime from the end of the main sequence to He-ignition set at log LHe/L⊙ = 1. HeCF: Full He-core flash (and subflashes) at the beginning of the core He-burning phase. τHeCB: lifetime of core He-burning, until 
. τeAGB: lifetime of the early AGB phase from the end of core helium burning to the first thermal pulse. : mass of the H-free core at the first thermal pulse (defined as those regions with XH< 10-4). τTP−AGB(M): lifetime of the star in the TP-AGB as a M-type star (NC/NO< 1). τTP−AGB(C): lifetime of the star in the TP-AGB as a carbon star (NC/NO> 1). #TP: number of thermal pulses on the AGB. Mf: final mass of the star. NC/NO: C/O ratio in number fraction at the end of the TP-AGB phase.
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