We investigate the hydrodynamics of three-dimensional classical Bondi-Hoyle accretion. A totally absorbing sphere of different sizes (1, 0.1 and 0.02 accretion radii) moves at different Mach numbers (0.6, 1.4, 3.0 and 10) relative to a homogeneous and slightly perturbed medium, which is taken to be an ideal, nearly isothermal, gas (#gamma#=1.01). We examine the influence of Mach number of the flow and size of the accretor upon the physical behaviour of the flow and the accretion rates. The hydrodynamics is modeled by the Piecewise Parabolic Method (PPM). The resolution in the vicinity of the accretor is increased by multiply nesting several 32"3-zone grids around the sphere, each finer grid being a factor of two smaller in zone dimensi...
The adiabatic shock produced by a compact object moving supersonically relative to a gas with unifor...
The morphology of adiabatic accretion flows with small non-zero specific angular momentum has been i...
Context. Isolated stellar-mass black holes accrete gas from their surroundings, often at supersonic ...
We investigate the hydrodynamics of three-dimensional classical Bondi-Hoyle accretion. A totally abs...
We investigate the hydrodynamics of three-dimensional classical Bondi-Hoyle accretion, especially th...
We prove that the sonic surface of axisymmetric meridional stationary flows is always attached to th...
The hydrodynamics of a variant of classical Bondi-Hoyle-Lyttleton accretion is investigated: a total...
In this paper, we discuss a two-dimensional numerical study of isothermal high Mach number Bondi-Hoy...
A second order Alternating Direction Implicit/Explicit computer code, or SADIE for short, has been d...
The Bondi-Hoyle formula gives the approximate accretion rate onto a point particle accreting from a ...
In this paper, we discuss a two-dimensional numerical study of isothermal high Mach number Bondi--Ho...
We present a new code for performing general-relativistic radiation-hydrodynamics simulations of acc...
International audienceBondi–Hoyle accretion configurations occur as soon as a gravitating body is im...
The instability of Bondi-Hoyle-Lyttleton accretion, observed in numerical simulations, is analyzed t...
Numerical simulations of hot accretion flow, both hydrodynamical and magnetohydrodynamical, have sho...
The adiabatic shock produced by a compact object moving supersonically relative to a gas with unifor...
The morphology of adiabatic accretion flows with small non-zero specific angular momentum has been i...
Context. Isolated stellar-mass black holes accrete gas from their surroundings, often at supersonic ...
We investigate the hydrodynamics of three-dimensional classical Bondi-Hoyle accretion. A totally abs...
We investigate the hydrodynamics of three-dimensional classical Bondi-Hoyle accretion, especially th...
We prove that the sonic surface of axisymmetric meridional stationary flows is always attached to th...
The hydrodynamics of a variant of classical Bondi-Hoyle-Lyttleton accretion is investigated: a total...
In this paper, we discuss a two-dimensional numerical study of isothermal high Mach number Bondi-Hoy...
A second order Alternating Direction Implicit/Explicit computer code, or SADIE for short, has been d...
The Bondi-Hoyle formula gives the approximate accretion rate onto a point particle accreting from a ...
In this paper, we discuss a two-dimensional numerical study of isothermal high Mach number Bondi--Ho...
We present a new code for performing general-relativistic radiation-hydrodynamics simulations of acc...
International audienceBondi–Hoyle accretion configurations occur as soon as a gravitating body is im...
The instability of Bondi-Hoyle-Lyttleton accretion, observed in numerical simulations, is analyzed t...
Numerical simulations of hot accretion flow, both hydrodynamical and magnetohydrodynamical, have sho...
The adiabatic shock produced by a compact object moving supersonically relative to a gas with unifor...
The morphology of adiabatic accretion flows with small non-zero specific angular momentum has been i...
Context. Isolated stellar-mass black holes accrete gas from their surroundings, often at supersonic ...