Fig. D.2.

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I propose two possible scenarios in which Hα emission could be generated: 1) an emission region locked with M dwarf, co-orbiting the WD, though 1.7 times farther away from the WD; 2) an emission region originating from material falling into the WD, either through free-fall or by being magnetically channeled. Both diagrams are shown at the ascending node, where the radio pulses occur.
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