Issue |
EAS Publications Series
Volume 64, 2013
Setting a New Standard in the Analysis of Binary Stars
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Page(s) | 59 - 66 | |
Section | Setting a New Standard in the Analysis of High-Mass Binary Stars | |
DOI | https://doi.org/10.1051/eas/1364008 | |
Published online | 25 February 2014 |
Setting a New Standard in the Analysis of Binary Stars
K. Pavlovski, A. Tkachenko and G. Torres (eds)
EAS Publications Series, 64 (2013) 59-66
K. Pavlovski, A. Tkachenko and G. Torres (eds)
EAS Publications Series, 64 (2013) 59-66
Interacting winds in massive binaries
Institut d'Astrophysique & de Géophysique, Université de Liège, Belgium
Massive stars feature highly energetic stellar winds that interact whenever two such stars are bound in a binary system. The signatures of these interactions are nowadays found over a wide range of wavelengths, including the radio domain, the optical band, as well as X-rays and even γ-rays. A proper understanding of these effects is thus important to derive the fundamental parameters of the components of massive binaries from spectroscopic and photometric observations.
© EAS, EDP Sciences, 2014