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Table 4
Stellar wind parameters.
T | v ∞ | β | R ∗ | Ṁ | X(C) | X(N) | X(O) | |
kK | km s-1 | R ⊙ | 10-6 M⊙ yr-1 | |||||
|
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This work | 401 | 2300 | 1 | 17.3 | 3.5 | 6.00 × 10-4 | 7.7 × 10-3 | 3.05 × 10-3 |
|
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Bouret et al. (2012) | 40 | 2300 | 0.9 | 17.3 | 2.00 | 2.86 × 10-4 | 1.05 × 10-2 | 1.30 × 10-3 |
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Pauldrach et al. (2012) | 39 | 2100 | – | 19 | 13.7 | 8.2 × 10-3 | 9.13 × 10-3 | 1.14 × 10-3 |
Notes. The CNO abundances are given as mass fractions. Note that Pauldrach et al. (2012) did not assume a β-law for the wind velocity, but performed a full hydrodynamical computation of the wind.
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