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Table 4
Stellar and wind parameters adopted in the computation of the X-ray opacities.
| Primary | Secondary | |
|---|---|---|
| Teff (K) | 34000 | 28000 |
| R(R⊙) | 15.7 | 21.8 |
| υ∞ (km s−1) | 2450 | 2450 |
![$\[\dot{M}\]$](/articles/aa/full_html/2024/06/aa48721-23/aa48721-23-eq48.png){kind=small} (M⊙ yr−1) |
9.2 × 10−7 | 3.3 × 10−7 |
| β | 1.03 | 1.08 |
| ϵC/ϵC,⊙ | 0.38 | 0.07 |
| ϵN/ϵN,⊙ | 1.95 | 10.6 |
| ϵO/ϵO,⊙ | 1.50 | 0.16 |
Notes. The parameters are from Raucq et al. (2016), except for the radii taken from the combined photometric and astrometric analysis of Rauw et al. (2019). The mass-loss rates were computed using the formalism of Muijres et al. (2012).
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