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Constraining the emission geometry and mass of the white Dwarf Pulsar AR Sco
(North-West University (South Africa), 2020)
Marsh et al. (2016) detected radio and optical pulsations from the binary system AR Scorpii (AR Sco). This system, with an orbital period of 3.55 h, is composed of a cool, low-mass M-dwarf and a white dwarf with a spin ...