Table 3
Adopted model parameters and predicted wind properties.
| Model parameters | Wind properties | |||||||||
| L | M | Teff | R | ZCNO | ṀV | Abund. | Ṁ | ν∞ | νesc | β |
| log (L⊙) | M⊙ | kK | R⊙ | log (M⊙/yr) | pattern | log (M⊙/yr) | km s-1 | km s-1 | ||
|
|
||||||||||
| 5.50 | 30.0 | 50.0 | 7.5 | 0.04 | –5.496 | – | – | – | – | – |
| 0.02 | –5.752 | – | – | – | – | – | ||||
| 0.002 | –6.602 | – | – | – | – | – | ||||
| 40.0 | 11.7 | 0.04 | –5.484 | – | – | – | – | – | ||
| 0.02 | –5.740 | – | – | – | – | – | ||||
| 0.002 | –6.590 | 3 | –6.908 | 2330 | 852 | 0.72 | ||||
| 0.002 | –6.590 | 4 | –6.913 | 2060 | 900 | 0.64 | ||||
| 30.0 | 20.9 | 0.04 | –5.771 | 2 | –6.788 | 5406 | 647 | 1.12 | ||
| 0.02 | –6.027 | 1 | –6.702 | 2100 | 644 | 0.78 | ||||
| 0.002 | –6.877 | 1: | –6.766 | 1150 | 644 | 0.66 | ||||
| 3 | –6.786 | 1193 | 646 | 0.64 | ||||||
| 20.0 | 47.0 | 0.04 | –5.510 | 2: | –6.586 | 956 | 436 | 0.67 | ||
| 0.02 | –5.765 | 1: | –6.860 | 2750 | 434 | 1.23 | ||||
| 0.002 | –6.615 | 1: | –6.818 | 1550 | 434 | 0.84 | ||||
| 2: | –6.722 | 1126 | 436 | 0.72 | ||||||
| 5.75 | 45.0 | 50.0 | 10.0 | 0.04 | –5.179 | – | – | – | – | – |
| 0.02 | –5.435 | – | – | – | – | – | ||||
| 0.002 | –6.285 | – | – | – | – | – | ||||
| 40.0 | 15.6 | 0.04 | –5.167 | – | – | – | – | – | ||
| 0.02 | –5.422 | – | – | – | – | – | ||||
| 0.002 | –6.272 | 1 | –6.571 | 2080 | 875 | 0.67 | ||||
| 2 | –6.588 | 2204 | 875 | 0.71 | ||||||
| 3 | –6.601 | 2377 | 875 | 0.70 | ||||||
| 30.0 | 27.8 | 0.04 | –5.454 | 3 | –6.488 | 3130 | 666 | 0.84 | ||
| 0.02 | –5.709 | – | – | – | – | – | ||||
| 0.002 | –6.559 | 1 | –6.488 | 1060 | 665 | 0.66 | ||||
| 2: | –6.502 | 900 | 665 | 0.60 | ||||||
| 4 | –6.729 | 4800 | 723 | 0.95 | ||||||
| 20.0 | 62.4 | 0.04 | –5.193 | 1 | –6.490 | 2030 | 450 | 0.86 | ||
| 3 | –6.610 | 2694 | 450 | 1.09 | ||||||
| 0.02 | –5.449 | 1 | –6.399 | 1250 | 450 | 0.69 | ||||
| 2: | –6.299 | 950 | 450 | 0.80 | ||||||
| 3 | –6.416 | 1412 | 450 | 0.81 | ||||||
| 0.002 | –6.299 | – | – | – | – | – | ||||
| 6.00 | 65.0 | 50.0 | 13.3 | 0.04 | –4.840 | – | – | – | – | – |
| 0.02 | –5.096 | – | – | – | – | – | ||||
| 0.002 | –5.946 | – | – | – | – | – | ||||
| 40.0 | 20.8 | 0.04 | –4.828 | – | – | – | – | – | ||
| 0.02 | –5.084 | – | – | – | – | – | ||||
| 0.002 | –5.934 | 1 | –6.305 | 2500 | 863 | 0.72 | ||||
| 2 | –6.318 | 2400 | 863 | 0.71 | ||||||
| 3 | –6.352 | 2752 | 863 | 0.75 | ||||||
| 30.0 | 37.0 | 0.04 | –5.115 | 1 | –6.212 | 4740 | 661 | 1.06 | ||
| 0.02 | –5.371 | 1: | –6.160 | 2450 | 661 | 0.78 | ||||
| 0.002 | –6.221 | 2 | –6.215 | 1305 | 660 | 0.64 | ||||
| 3: | –6.230 | 1205 | 659 | 0.63 | ||||||
| 4 | –6.301 | 2500 | 736 | 0.76 | ||||||
| 20.0 | 83.3 | 0.04 | –4.854 | 1 | –6.132 | 1625 | 449 | 0.80 | ||
| 2: | –6.130 | 1350 | 449 | 0.71 | ||||||
| 3: | –6.084 | 905 | 449 | 0.65 | ||||||
| 0.02 | –5.110 | 1: | –6.236 | 1950 | 449 | 0.96 | ||||
| 2: | –6.144 | 1450 | 449 | 0.82 | ||||||
| 0.002 | –5.960 | 1 | –6.172 | 1250 | 449 | 0.76 | ||||
| 2: | –6.309 | 1620 | 449 | 0.87 | ||||||
| 6.25 | 80.0 | 50.0 | 17.8 | 0.04 | –4.410 | – | – | – | – | – |
| 0.02 | –4.666 | – | – | – | – | – | ||||
| 0.002 | –5.516 | – | – | – | – | – | ||||
| 40.0 | 27.8 | 0.04 | –4.398 | – | – | – | – | – | ||
| 0.02 | –4.653 | – | – | – | – | – | ||||
| 0.002 | –5.503 | 1 | –5.962 | 2310 | 711 | 0.76 | ||||
| 2 | –6.004 | 2616 | 709 | 0.80 | ||||||
| 3: | –6.013 | 2721 | 709 | 0.81 | ||||||
| 4 | –6.137 | 3400 | 840 | 0.75 | ||||||
| 30.0 | 49.3 | 0.04 | –4.685 | 2 | –5.943 | 5400 | 554 | 1.16 | ||
| 0.02 | –4.941 | 2: | –5.837 | 2274 | 552 | 0.84 | ||||
| 3 | –5.843 | 2000 | 552 | 0.77 | ||||||
| 0.002 | –5.791 | 2 | –5.879 | 1483 | 552 | 0.74 | ||||
| 4 | –5.927 | 1667 | 669 | 0.65 | ||||||
| 20.0 | 111.0 | 0.04 | –4.422 | 1 | –5.786 | 1110 | 382 | 0.74 | ||
| 2: | –5.877 | 1567 | 382 | 0.81 | ||||||
| 3: | –5.761 | 1240 | 382 | 0.81 | ||||||
| 0.02 | –4.678 | 1 | –5.978 | 2000 | 382 | 0.91 | ||||
| 2 | –5.888 | 1615 | 381 | 0.93 | ||||||
| 3: | –5.929 | 1600 | 381 | 0.83 | ||||||
| 0.002 | –5.528 | – | – | – | – | – | ||||
Notes. Both the models for which a wind solution is achieved and those for which this is not the case are listed. The chemical compositions (Col. 7) correspond to the coding as given in Table 1. Typical errors on the theoretical mass-loss rates are 0.1–0.2 dex; the errors on the terminal velocities are ~30%.For models in which the abundance pattern is followed by a semi colon the errors are larger. The reference mass-loss rates ṀV are as given by Vink et al. (2001), if we employ ν∞ = 2.6 νesc. Beware that in order to compute ṀV we have set the value of ZCNO equal to the metallicity value Z, which is not intended by the ṀV-recipe, in which Z refers to the initial iron abundance. Small changes in the effective escape velocity from the stellar surface (Col. 10) are due to abundance effects on Γe.
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