Table 3
As in Table 2, but for the second grid of stellar models (grid (2) in Table 1).
| f | F0 | Amax | n c | MCZME | Duration [s] | |||
|
|
||||||||
| (a) | 10-5 | 3.78 | 86−87 | 0.16 | 3.52 M⊙ | 3.58 × 1013 | ||
| 0.01 | 4.30 | 86−87 | 0.23 | 4.54 M⊙ | 3.57 × 1013 | |||
| 0.02 | 4.27 | 86−87 | 0.23 | 5.19 M⊙ | 3.18 × 1013 | |||
| 0.035 | 4.34 | 86−87 | 0.24 | 5.58 M⊙ | 3.08 × 1013 | |||
|
|
||||||||
| (b) | 10-5 | 9.56 | 87−88 | 1.19 | 3.96 M⊙ | 4.04 × 1013 | ||
| 0.01 | 10.47 | 88−89 | 1.31 | 4.46 M⊙ | 3.78 × 1013 | |||
| 0.02 | 11.06 | 88−89 | 1.40 | 4.93 M⊙ | 3.21 × 1013 | |||
| 0.035 | 11.14 | 88−89 | 1.40 | 5.26 M⊙ | 2.89 × 1013 | |||
|
|
||||||||
| (c) | 10-5 | 48.05 | 89−92 | 3.08 | 3.94 M⊙ | 4.09 × 1013 | ||
| 0.01 | 72.14 | 89−94 | 3.65 | 4.15 M⊙ | 3.79 × 1013 | |||
| 0.02 | 68.27 | 91−94 | 3.57 | 4.80 M⊙ | 3.40 × 1013 | |||
| 0.035 | 125.44 | 92−98 | 4.29 | 5.23 M⊙ | 3.14 × 1013 | |||
Notes. Sets (a), (b), and (c) refer to the M = 20 M⊙ stellar models with Z = 10-4, 0.005, and 0.01, respectively. The overshooting parameter value used in the stellar evolution code is reported in the first column for each set of stellar models with a fixed initial metallicity.
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