Really focused stellar winds in X-ray binaries
Solar and Stellar Astrophysics
2015-06-05 v1 High Energy Astrophysical Phenomena
Abstract
We investigate the anisotropy of stellar winds in binaries to improve the models of accretion in high-mass X-ray binaries. We model numerically the stellar wind from a supergiant component of a binary in radial and three-dimensional radiation hydrodynamic approximation taking into account the Roche potential, Coriolis force, and radiative pressure in the continuum and spectral lines. The Coriolis force influences substantially the mass loss and thus also the accretion rate. The focusing of the stellar wind by the gravitational field of the compact companion leads to the formation of a gaseous tail behind the companion.
Cite
@article{arxiv.1205.2016,
title = {Really focused stellar winds in X-ray binaries},
author = {Petr Hadrava and Jan Čechura},
journal= {arXiv preprint arXiv:1205.2016},
year = {2015}
}
Comments
10 figures