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.
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Walder, R. 1993, PhD thesis, ETH Zürich
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© 1995 Springer Science+Business Media Dordrecht
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Walder, R. (1995). Simulations of Colliding Winds in 3 Dimensions. In: van der Hucht, K.A., Williams, P.M. (eds) Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution. International Astronomical Union / Union Astronomique Internationale, vol 163. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0205-6_92
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DOI: https://doi.org/10.1007/978-94-011-0205-6_92
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