No CrossRef data available.
Article contents
Simulations of colliding winds in 3 dimensions
Published online by Cambridge University Press: 07 August 2017
Abstract
The significance of 3D effects in simulating colliding winds in WR binaries is demonstrated for the examples V444 Cyg, HD 193793 and γ Vel. The effects decrease with increasing separation of the stars. A comparison with symbiotic systems is drawn and a simulation of the symbiotic system EG And is presented.
Keywords
- Type
- Session VII - Hydrodynamics and high-energy physics of colliding winds
- Information
- Copyright
- Copyright © Kluwer 1995