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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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.