Kinetic plasma simulations show the electron cyclotron maser instability can produce efficient, narrowband, partially linearly polarized radio emission under conditions inferred for white dwarf-M dwarf binaries.
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Unraveling the emission mechanism powering long period radio transients from interacting white dwarf binaries via kinetic plasma simulations
Kinetic plasma simulations show the electron cyclotron maser instability can produce efficient, narrowband, partially linearly polarized radio emission under conditions inferred for white dwarf-M dwarf binaries.