Table 1
Probabilities for the simulations with M ≈ 100 M⊙.
 interval
(104 K) |
# Simulations | Probability (%) | Partial probability (%) | Stellar mass (M⊙) |
|
|
||||
| 4.92–5.51 | 259 | 0.64 | 3.31 | 100 |
| 4.24–4.92 | 2410 | 5.95 | 30.80 | 50 |
| 3.70–4.24 | 3503 | 8.65 | 44.77 | 25 |
| 3.4–3.7 | 1653 | 4.08 | 21.12 | 20 |
| 0.2–3.4 | 32 677 | 80.68 | – | ≤20 |
Notes. The first column shows the 
interval in which
probabilities are computed; these ranges are also shown in Fig. 8. The second column gives the number of simulations in each
range. The third column
shows the probability of each range when the complete
set of simulations is considered. The fourth column shows the corresponding
probability when only the subset of simulations that can generate an
H ii region is considered. The last column lists the stellar mass
corresponding to the middle point of each temperature range.
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