A bow shock around a diskless polar cataclysmic variable requires persistent power exceeding accretion energy, pointing to a new magnetic energy-loss mechanism that may affect binary evolution.
C.et al.Cataclysmic Variables and AM CVn Binaries in SRG/eROSITA + Gaia: Volume Limited Samples, X-Ray Luminosity Func- tions, and Space Densities.Publ
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A persistent bow shock in a diskless magnetised accreting white dwarf
A bow shock around a diskless polar cataclysmic variable requires persistent power exceeding accretion energy, pointing to a new magnetic energy-loss mechanism that may affect binary evolution.