Open Access
Table 1.
Model parameters for three typical SNR-PWN systems.
| M1 | M2 | M3 | |
|---|---|---|---|
Pulsar spin-down power  (erg s−1) |
3.0 × 1038 | 3.0 × 1037 | 3.0 × 1036 |
| Pulsar spin-down timescale τ0 (yr) | 6.0 × 102 | 3.0 × 103 | 3.0 × 104 |
| Pulsar braking index | 3.0 | 3.0 | 3.0 |
| Ejecta energy Eej (erg) | 1051 | ||
| Ejecta mass Mej (M⊙) | 10 | ||
| Circumstellar medium density n0 (H cm−3) | 0.1 | ||
| Turbulence scale κT | 0.02 | ||
| Turbulent energy injection efficiency ηT | 0.075 | ||
| Magnetic energy injection efficiency ηB | 0.025 | ||
| Particle energy injection efficiency ηe | 0.90 | ||
| Particle injection spectrum low-energy index α1 | 1.5 | ||
| Particle injection spectrum high-energy index α2 | 2.6 | ||
| Particle injection spectrum break energy Eb (GeV) | 500 | ||
| Particle injection spectrum cut-off energy Ec (TeV) | 300 | ||
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