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Table 3.
Mass flux and speed of the companion star wind, and the corresponding power ratio (assuming a pulsar spin-down luminosity Lsd = 1035 erg/s).
| ṁc,w (M⊙/yr) | (a) | (b) |
|---|---|---|
| 4.5 × 10−10 | 9 × 10−10 | |
| (0) | ||
| vc, w = 60 km/s | ||
| ξc, rot ∼ 0.12 | ϵ = 1.13 × 10−4 | ϵ = 2.26 × 10−4 |
| ξc, grav ∼ 0.4 | ||
| (1) | ||
| vc, w = 100 km/s | ||
| ξc, rot ∼ 0.2 | ϵ = 3.14 × 10−4 | ϵ = 6.29 × 10−4 |
| ξc, grav ∼ 0.67 | ||
| (2) | ||
| vc, w = 150 km/s | ||
| ξc, rot ∼ 0.3 | ϵ = 7.08 × 10−4 | ϵ = 1.41 × 10−3 |
| ξc, grav ∼ 1 | ||
| (3) | ||
| vc, w = 200 km/s | ||
| ξc, rot ∼ 0.4 | ϵ = 1.25 × 10−3 | ϵ = 2.51 × 10−3 |
| ξc, grav ∼ 1.33 | ||
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