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Heat conduction and colliding winds in Wolf-Rayet binaries

Published online by Cambridge University Press:  25 May 2016

Simin M. Motamen ,
Rolf Walder  and
Doris Folini
Simin M. Motamen
Affiliation:
Seminar für angewandte Mathematik, ETH Zürich, Switzerland
Rolf Walder
Affiliation:
Institut für Astronomie, ETH Zürich, Switzerland
Doris Folini
Affiliation:
Institut für Astronomie, ETH Zürich, Switzerland

Abstract

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We numerically investigate the impact of heat conduction by thermal electrons on the physics of colliding winds by means of a 1D model problem. Compared to ideal flows, the hot plasma has significantly lower temperatures and has both a high- and low-density component. Consequently, the shocks in WR binaries become generally more radiative and the emitted X-ray spectrum is softer, shows more emission lines, and is a composite of the emission from high- and low density regions.

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. 378 - 379
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Spitzer, L. 1965, Physics of Fully Ionized Gases (New York: Interscience Publ.)Google Scholar
Dai, W., Woodward, P.R. 1998, Journ. Comp. Phys. 142, 182 Google Scholar
Myasnikov, A.V., Zhekov, S.A. 1998, MNRAS 300, 686 Google Scholar
Walder, R., Folini, D. 1996, A&A 315, 265 Google Scholar