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Current Problems for X-ray Emission from Radio Jets

D. E. Harris
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Abstract

A list is presented of known extragalactic radio jets which also have associated X-ray emission. The canonical emission processes for the production of X-rays are reviewed and the sources are categorized on the basis of our current understanding. Although it seems clear that the X-ray emission is non-thermal, the two competing processes, synchrotron and inverse Compton emissions, arise from extremely high energy (synchrotron) or extremely low energy (beaming models with IC emission), relativistic electrons. Only synchrotron self-Compton emission from a few hotspots provides information on the `normal' energy range of the electrons responsible for the observed radio emission.

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D. E. Harris. 2000-12-17. Current Problems for X-ray Emission from Radio Jets. https://arxiv.org/abs/astro-ph/0012374

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