Table 1.
Parameters of the models.
| Name | Md | Ma | q | P | a | e | Jorb | vpe | vap | v∞ | v∞/vpe | v∞/vap | Ωspin | RL, 1|pe | Rd | Rsink | Teff | Ṁd | mg |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| – | M⊙ | M⊙ | – | yr | AU | – | m2 kg s−1 | km s−1 | km s−1 | km s−1 | – | – | s−1 | R⊙ | R⊙ | R⊙ | K | M⊙ yr−1 | M⊙ |
| Q2e0 | 1.2 | 0.6 | 2 | 5.96 | 4.00 | 0 | 9.51 × 1045 | 19.98 | 19.98 | 15.1 | 0.76 | 0.76 | 3.34 × 10−8 | 378.6 | 330 | 27.6 | 3240 | 1.5 × 10−5 | 9.6 × 10−10 |
| Q2e02 | 1.2 | 0.6 | 2 | 8.33 | 5.00 | 0.2 | 1.04 × 1046 | 21.89 | 14.59 | 15.1 | 0.69 | 1.03 | 3.66 × 10−8 | 376.3 | 330 | 27.2 | 3240 | 1.5 × 10−5 | 1.2 × 10−9 |
| Q2e04 | 1.2 | 0.6 | 2 | 12.83 | 6.66 | 0.4 | 1.13 × 1046 | 23.64 | 10.13 | 15.1 | 0.64 | 1.49 | 3.95 × 10−8 | 371.7 | 330 | 26.9 | 3240 | 1.5 × 10−5 | 1.6 × 10−9 |
| Q2e06 | 1.2 | 0.6 | 2 | 23.57 | 10.00 | 0.6 | 1.20 × 1046 | 25.28 | 6.32 | 15.1 | 0.60 | 2.39 | 4.22 × 10−8 | 365.9 | 330 | 26.8 | 3240 | 1.5 × 10−5 | 2.4 × 10−9 |
| Q2e08 | 1.2 | 0.6 | 2 | 66.66 | 20.00 | 0.8 | 1.28 × 1046 | 26.81 | 2.98 | 15.1 | 0.56 | 5.07 | 4.48 × 10−8 | 362.5 | 330 | 138.9 | 3240 | 1.5 × 10−5 | 4.8 × 10−9 |
| Q2e06v1 | 1.2 | 0.6 | 2 | 23.57 | 10.00 | 0.6 | 1.20 × 1046 | 25.28 | 6.32 | 6.0 | 0.24 | 0.95 | 4.22 × 10−8 | 365.9 | 330 | 26.8 | 3240 | 1.5 × 10−5 | 2.4 × 10−9 |
| MMe05 | 3.0 | 1.5 | 2 | 5.27 | 5.00 | 0.5 | 3.64 × 1046 | 48.95 | 16.32 | 14.2 | 0.31 | 0.93 | 0 | 231.3 | 200 | 16.7 | 2430 | 1.5 × 10−5 | 1.6 × 10−9 |
Notes. The first column corresponds to the name of the model. Md and Ma are the masses of the donor and accretor star, and q is the mass ratio. P, a, and e are the orbital period, semi-major axis, and eccentricity. Jorb is the initial orbital angular momentum of the binary. vpe and vap are the orbital velocities at periastron and apastron, respectively, and v∞ is the terminal velocity of the wind. Ωspin is the spin angular velocity of the donor star. RL, 1|pe is the Roche-lobe radius of the primary star at periastron. Rd is the radius of the donor star and Rsink is the radius of the sink particle representing the companion star. Teff is the effective temperature of the primary star that also determines the initial temperature of the wind particles. Ṁd is the mass-loss rate of the donor star and mg is the SPH particle mass.
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