TXS 0506+056's delayed radio flare is modeled as the jet running into three parsec-scale electron clouds, reproducing frequency-dependent radio peak delays.
The additional, contributing electron population has a bulk Lorentz factor of 10, magnetic field strength of 0.03 G, and a radius of 2000 light days
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An Evolving Leptonic Jet Model for Delayed Radio Flares in Neutrino Blazars
TXS 0506+056's delayed radio flare is modeled as the jet running into three parsec-scale electron clouds, reproducing frequency-dependent radio peak delays.