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3D hydrodynamic simulations of colliding winds in V444 Cygni

Published online by Cambridge University Press:  25 May 2016

Julian M. Pittard  and
Ian R. Stevens
Julian M. Pittard
Affiliation:
The University of Birmingham, Edgbaston, Birmingham B15 2TT, UK
Ian R. Stevens
Affiliation:
The University of Birmingham, Edgbaston, Birmingham B15 2TT, UK

Abstract

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We report on recent developments in simulating colliding wind X-ray emission, and present a 3D model of the WR binary V444 Cyg (WN5+O6) which self-consistently includes radiative driving.

Type
Part 3. Interaction of Wolf-Rayet stars and other hot massive stars with their environment: colliding winds and ring nebulae
Information
Symposium - International Astronomical Union , Volume 193: Wolf-Rayet Phenomena in Massive Stars and Starburst Galaxies , 1999 , pp. 386 - 387
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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