A new particle-dynamics emission code reproduces AR Sco's spectral energy distribution in a magnetic mirror model, constraining the white dwarf magnetic field to roughly 250-300 MG.
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Modelling the multi-wavelength emission and polarisation signatures of the novel white-dwarf pulsar system AR Sco
A new particle-dynamics emission code reproduces AR Sco's spectral energy distribution in a magnetic mirror model, constraining the white dwarf magnetic field to roughly 250-300 MG.