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 …

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 …

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

We investigate the structure and X-ray emission from the colliding stellar winds in massive
star binaries. We find that the opening angle of the contact discontinuity (CD) is …

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 …

Context. In massive binaries, the powerful stellar winds of the two stars collide, leading to the
formation of shock-dominated environments that can be modeled only in 3D. Aims. We …

Stellar winds shape the evolution of stars through the loss of mass. In binary systems, they
also shape the stars' evolution by modifying the orbit. In this paper, we use hydrodynamic …

Massive binary systems are excellent laboratories for studying stellar winds. The powerful
collision of the winds unleashes a broad spectrum of emission revealing the interesting …

The dynamics of the wind–wind collision in massive stellar binaries are investigated using
3D hydrodynamical models which incorporate gravity, the driving of the winds, the orbital …

Some red giant envelopes present spiral structures (seen either in dust-scattered stellar
continuum or in molecular line emission), the most striking example probably being AFGL …