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Simulations of colliding winds in 3 dimensions

Published online by Cambridge University Press:  07 August 2017

Rolf Walder
Rolf Walder*
Affiliation:
Institut für Astronomie, ETH-Zentrum, 8092 Zürich, Switzerland

Abstract

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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

stars: Wolf-Rayethydrodynamicscolliding windsindividual: V444 CygHD 193793γ Velsymbiotic systemsindividual: EG And
Type
Session VII - Hydrodynamics and high-energy physics of colliding winds
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 420 - 424
Copyright
Copyright © Kluwer 1995 

References

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Walder, R. 1993, PhD thesis, ETH Zürich Google Scholar