Research Article
Pulsar-Driven Jets in Supernovae, Gamma-Ray Bursts, and the Universe
Table 2
15
DD-formed pulsar processes.
| Process | Timespan
|
| Bi-lobed to spheroidal CE | ~−2,000? years | Chandrasekhar-mass WD formed | ~−2? seconds | DD core-collapse to 2 ms pulsar | ~−? s | Gamma-ray burst (GRB) | ~ ~100? s | Pulsed GRB afterglow | ~ day | Ejection spindown phase, | years | Transition to | years | GR-dominated spindown | ? years | Broadly beamed pulsations | years | Plasma depleted | years | Cas A-type thermal X-ray source | years | Magnetic dipole-dominated spindown | years |
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