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...

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Bibliographic Details
Main Authors: Araudo Anabella T., Bosch-Ramon Valentí, Romero Gustavo E.
Format: Article
Language:English
Published: EDP Sciences 2013-12-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20136105014