- Abstract:
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The high-mass microquasar Cygnus X-3 has been recently detected in a flaring state by the gamma-ray satellites Fermi and Agile. In the present contribution, we study the high-energy emission from Cygnus X-3 through a model based on the interaction of clumps from the Wolf-Rayet wind with the jet. The clumps inside the jet act as obstacles in which shocks are formed leading to particle acceleration and non-thermal emission. We model the high energy emission produced by the interaction of one cl...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
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(pdf, 118.8KB)
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- Publisher:
- Proceedings of Science Publisher's website
- Volume:
- SESSION P6
- URN:
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pubs:d8025711-e050-4d96-b861-ddb7e5163c6e
- Source identifiers:
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519321
- Local pid:
- info:fedora/pubs:519321
- Keywords:
- Copyright holder:
- Anabella Araudo et al.
- Notes:
- This article is distributed under the terms of a Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (https://creativecommons.org/licenses/by-nc-nd/4.0/)
Conference
Transient gamma-ray emission from Cygnus X-3
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