Simulations find nested bow shocks around an engulfed neutron star enhance drag force 10-100 times over Bondi-Hoyle-Lyttleton and allow force reversal based on envelope conditions.
J.] 10.3847/1538-4357/ab89aa , https://ui.adsabs.harvard.edu/abs/2020ApJ...894..147C 894, 147
2 Pith papers cite this work, alongside 30 external citations. Polarity classification is still indexing.
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2D general-relativistic simulations of Bondi-Hoyle-Lyttleton accretion onto a Kerr black hole in a common envelope yield analytical fits for mass/momentum accretion rates and bremsstrahlung luminosity as functions of spin, Mach number, and density gradient.
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Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
Simulations find nested bow shocks around an engulfed neutron star enhance drag force 10-100 times over Bondi-Hoyle-Lyttleton and allow force reversal based on envelope conditions.
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Relativistic Common-envelope Dynamics of a Stellar-mass Black Hole II: Kerr Black Hole
2D general-relativistic simulations of Bondi-Hoyle-Lyttleton accretion onto a Kerr black hole in a common envelope yield analytical fits for mass/momentum accretion rates and bremsstrahlung luminosity as functions of spin, Mach number, and density gradient.