Conference item
Transient gamma-ray emission from Cygnus X-3
- 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...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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Authors
Bibliographic Details
- Publisher:
- Proceedings of Science Publisher's website
- Journal:
- 25th Texas Symposium on Relativistic Astrophysics - TEXAS 2010 Journal website
- Volume:
- SESSION P6
- Host title:
- 25th Texas Symposium on Relativistic Astrophysics
- Publication date:
- 2010-12-06
- Source identifiers:
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519321
Item Description
- Keywords:
- Pubs id:
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pubs:519321
- UUID:
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uuid:d8025711-e050-4d96-b861-ddb7e5163c6e
- Local pid:
- info:fedora/pubs:519321
- Deposit date:
- 2016-07-26
Terms of use
- Copyright holder:
- Anabella Araudo et al
- Copyright date:
- 2010
- 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/)
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