We carry out a numerical experiment for ejecting winds in a massive colliding-wind binary
system and quantify the accretion on to the secondary star under different primary mass-loss …

We run a numerical experiment ejecting stellar winds in a very massive binary system
measuring the properties of the resulting colliding wind structure and accreted mass onto the …

Using fully three-dimensional hydrodynamic simulations, we investigate the effect of the
Coriolis force on the hydrodynamic and observable properties of colliding-wind binary …

Gravitationally focused wind accretion in binary systems consisting of an evolved star with a
gaseous envelope and a compact accreting companion is a possible mechanism to explain …

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 …

Binary stars often move through an ambient medium from which they accrete material and
angular momentum, as in triple-star systems, star-forming clouds, young globular clusters …

Using 3D radiation-hydrodynamic simulations and analytic theory, we study the orbital
evolution of asymptotic giant branch (AGB) binary systems for various initial orbital …

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 …

We investigate further the dynamics of colliding winds in hot-star binary systems, by
concentrating in this paper on the effects of the radiation pressure of both stars on the …

ABSTRACT I have run hydrodynamic simulations that follow the colliding wind structure of
the massive binary system HD 166734 along its binary orbit. I show that close to periastron …