Gamma-ray emission from early-type stars interacting with AGN jets
We study the interaction of early-type stars with the jets of active galactic nuclei. A bow-shock will form as a consequence of the interaction of the jet with the winds of stars and particles can be accelerated up to relativistic energies in these shocks. We compute the non-thermal radiation produc...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
EDP Sciences
2013-12-01
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Series: | EPJ Web of Conferences |
Online Access: | http://dx.doi.org/10.1051/epjconf/20136105014 |