arXiv · astro-ph/9906111
Internal shocks in blazar jets
Abstract
The discovery of strong gamma-ray and hard X-ray emission and the results from various multifrequency campaigns have disclosed new aspects of the blazar phenomenology, leading to a much more robust understanding of the mechanisms underlying their emission, and offering clues for the energetics of their relativistic jets. I review these aspects, and propose that all the diversity in the blazar phenomenology depends on only one parameter. I also suggest that some of the blazar characteristics can be explained by the internal shock scenario, as proposed to explain the emission from gamma-ray bursts.
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Gabriele Ghisellini. 1999-06-07. Internal shocks in blazar jets. https://doi.org/10.1002/1521-3994(199908)320%3A4%2F5%3C232%3A%3Aaid-asna232%3E3.0.co%3B2-b
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