Kavli Affiliate: Roger Romani | Summary:We present a model for pulsar filaments – a class of narrow X-ray nebulae misaligned with the proper motion, powered by pulsar-generated $e^pm$. We suggest that cosmic ray-enhanced turbulence drives pitch-angle scattering and dominates $e^pm$ motion along the filament; highly amplified magnetic fields are not required. A simulation built on […]
Continue.. A Physical Model of Pulsar X-ray Filaments