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X-rays from colliding winds in massive binaries

Published online by Cambridge University Press:  28 July 2017

Yaël Nazé Open the ORCID record for Yaël Nazé [Opens in a new window]  and
Gregor Rauw
Yaël Nazé
Affiliation:
FNRS/Université de Liège, Belgium, email: [email protected]
Gregor Rauw
Affiliation:
FNRS/Université de Liège, Belgium, email: [email protected]
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Abstract

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In a massive binary, the strong shock between the stellar winds may lead to the generation of bright X-ray emission. While this phenomenon was detected decades ago, the detailed study of this emission was only made possible by the current generation of X-ray observatories. Through dedicated monitoring and observations at high resolution, unprecedented information was revealed, putting strong constraints on the amount and structure of stellar mass-loss.

Keywords

X-rays: starsstars: early-typestars: windsstars: binaries
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S329: The Lives and Death-Throes of Massive Stars , November 2016 , pp. 359 - 360
Copyright
Copyright © International Astronomical Union 2017 

References

Rauw, G. & Nazé, Y., 2016, Ad. Sp. Research, 58, 761 Google Scholar