Table A.7
Parameters of the atmosphere models for the advanced phases tested in Sect. 5.2.
| M M⊙ | Teff K | log g | log(L/L⊙) | R R⊙ | ![$\[\log~ \dot{M}\]$](/articles/aa/full_html/2025/06/aa54421-25/aa54421-25-eq22.png) |
v∞ km s−1 | age Myr | H | He | C | N | O |
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Z = 0.1 Z⊙ | ||||||||||||
| 78.7 | 60571 | 4.01 | 6.403 | 15.20 | −4.23 | 2254 | 2.55 | 0.236 | 0.763 | 1.484 10−5 | 8.308 10−4 | 4.337 10−6 |
| 66.7 | 103323 | 4.83 | 6.439 | 5.20 | −3.94 | 4546 | 2.75 | 0.097 | 0.902 | 1.629 10−5 | 8.295 10−4 | 3.945 10−6 |
| 81.8 | 102201 | 4.78 | 6.558 | 6.10 | −3.84 | 3013 | 2.55 | 0.057 | 0.942 | 1.735 10−5 | 8.285 10−4 | 3.659 10−6 |
| Z = 0.01 Z⊙ | ||||||||||||
| 77.0 | 72384 | 4.32 | 6.393 | 10.10 | −4.23 | 2707 | 2.55 | 0.220 | 0.780 | 1.474 10−6 | 8.716 10−5 | 3.631 10−7 |
| 61.8 | 134223 | 5.28 | 6.410 | 3.00 | −3.99 | 3993 | 2.75 | 0.064 | 0.936 | 9.807 10−7 | 8.776 10−5 | 3.215 10−7 |
| 79.0 | 135932 | 5.28 | 6.538 | 3.37 | −3.88 | 4060 | 2.55 | 0.052 | 0.948 | 2.148 10−6 | 8.643 10−5 | 3.047 10−7 |
Notes. Columns are mass of the corresponding model according to stellar evolution rounded up to the first decimal, effective temperature, surface gravity, luminosity, radius, mass-loss rate, wind terminal velocity, age, and surface abundances of H, He, C, N, and O given in mass fraction. For each mass, the lines of this table correspond to the characteristics of the models marked as crosses in Fig. 1).
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