Chandra observations of CTA 1 PWN show jet/torus morphology, constrain pulsar velocity to ≲200 km/s, and model low magnetic field with PeV electron cutoff in a young low-efficiency nebula.
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Refined Crab nebula polarization is 27.7 ± 4.9% at 127.2 ± 5.1 degrees in 19-64 keV, with a new pulsar-based phase recovery method enabling inclusion of 95% of GPS-off data for stronger phase-resolved constraints.
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Chandra X-ray Observations of the Pulsar Wind Nebula within CTA 1
Chandra observations of CTA 1 PWN show jet/torus morphology, constrain pulsar velocity to ≲200 km/s, and model low magnetic field with PeV electron cutoff in a young low-efficiency nebula.
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Refined Constraints on the Hard X-ray Polarization of the Crab Pulsar and Nebula Derived from an Extended XL-Calibur Dataset
Refined Crab nebula polarization is 27.7 ± 4.9% at 127.2 ± 5.1 degrees in 19-64 keV, with a new pulsar-based phase recovery method enabling inclusion of 95% of GPS-off data for stronger phase-resolved constraints.