Issue |
EAS Publications Series
Volume 13, 2004
Evolution of Massive Stars, Mass Loss and Winds
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Page(s) | 293 - 316 | |
DOI | https://doi.org/10.1051/eas:2004058 | |
Published online | 15 November 2004 |
Evolution of Massive Stars, Mass Loss and Winds
M. Heydari-Malayeri, Ph. Stee and J.-P. Zahn (eds)
EAS Publications Series, 13 (2004) 293-316
M. Heydari-Malayeri, Ph. Stee and J.-P. Zahn (eds)
EAS Publications Series, 13 (2004) 293-316
Massive binaries and colliding winds
Institut d'Astrophysique et de Géophysique, Université de Liège, Allée du 6 Août 17, Bât B5c, 4000 Liège (Sart-Tilman), Belgium
In this contribution, I review recent results from observational investigations of early-type binaries of spectral types O and Wolf-Rayet. These studies aim at an accurate determination of fundamental parameters such as masses and radii of the most massive stars. In addition, multi-wavelength analyses of wind collisions in massive binaries provide constraints on the properties of stellar winds of massive stars and shock physics of cosmic plasmas.
© EAS, EDP Sciences, 2004