In the framework of Euler flows, I present simulations of wind accretion in well separated
binaries for three different cases: Cygnus X-3, a high mass X-ray binary (see eg Schmutz et …

About half of the binary systems are close enough to each other for mass to be exchanged
between them at some point in their evolution, yet the accretion mechanism in wind …

Three-dimensional hydrodynamic calculations are performed in order to investigate mass
transfer in a close binary system, in which one component undergoes mass loss through a …

The 3D flow structure of wind accretion in a binary system is computed numerically using
SPH, taking into account binary rotation as well as wind acceleration. In the adiabatic γ= 1.5 …

Smoothed particle hydrodynamics (SPH) is used to estimate accretion rates of mass, linear
and angular momentum in a binary system where one component undergoes mass loss …

I calculate the specific angular momentum of mass accreted by a binary system embedded
in the dense wind of a mass-losing asymptotic giant branch star. The accretion flow is of the …

Aims. We have developed a new code for the three-dimensional time-dependent raditation
hydrodynamic simulation of the stellar wind in interacting binaries to improve models of …

We present three-dimensional hydrodynamic calculations of mass transfer in an interacting
binary system in which one component undergoes mass loss through a wind, and does so …

Binary systems consisting of a secondary accreting form a wind-emitting primary are
ubiquitous in astrophysics. The phenomenology of such Bondi–Hoyle–Lyttleton (BHL) …

We perform numerical simulations to investigate the stellar wind from interacting binary
stars. Our aim is to find analytical formulae describing the outflow structure. In each binary …