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.
galpy: A python Library for Galactic Dynamics.Astrophys
2 Pith papers cite this work. Polarity classification is still indexing.
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Luminous quasars at z~5-6 show a high fraction of extreme [O III] outflows with velocities up to 8400 km/s and kinetic powers up to 2.6x bolometric luminosity, far exceeding lower-redshift samples and implying efficient early quenching.
citing papers explorer
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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.
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Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
Luminous quasars at z~5-6 show a high fraction of extreme [O III] outflows with velocities up to 8400 km/s and kinetic powers up to 2.6x bolometric luminosity, far exceeding lower-redshift samples and implying efficient early quenching.