Radio Emission from Pulsar Wind Nebulae Without Surrounding Supernova Ejecta: Application to FRB 121102
Z. G. Dai et al 2017 ApJL 838 L7
Rapidly rotating, strongly magnetized pulsars without any surrounding supernova ejecta could repeatedly produce fast radio bursts via synchrotron radio emission from non-relativistic pulsar wind nebulae.