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.
A.et al.TESS Photometry of AM Her and AR UMa: Binary Parameters, Cyclotron Emission Modeling, and Mass Transfer Duty Cycles
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
fields
astro-ph.SR 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
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.