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2008MNRAS.388.1047P - Mon. Not. R. Astron. Soc., 388, 1047-1061 (2008/August-2)
A 3D dynamical model of the colliding winds in binary systems.
PARKIN E.R. and PITTARD J.M.
Abstract (from CDS):
As an example application, we simulate the X-ray emission from hypothetical O+O and WR+O star binaries, and describe a method of ray tracing through the 3D spiral structure to account for absorption by the circumstellar material in the system. Such calculations may be easily adapted to study observations at wavelengths ranging from the radio to γ-ray.
Abstract Copyright: © 2008 The Authors. Journal compilation © 2008 RAS
Journal keyword(s): hydrodynamics - methods: numerical - binaries: general - stars: early-type - stars: winds, outflows - X-rays: stars
Errata: erratum vol. 403, p. 2176 (2010)
Simbad objects: 23
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