Synthetic radio maps of a runaway star bowshock show that free-free emission outshines synchrotron emission and that internal Faraday rotation makes polarization angles unreliable tracers of the magnetic field at 1.4 GHz.
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Radio polarization from runaway star bowshocks-I. The general case
Synthetic radio maps of a runaway star bowshock show that free-free emission outshines synchrotron emission and that internal Faraday rotation makes polarization angles unreliable tracers of the magnetic field at 1.4 GHz.