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Some Aspects of Inverse Compton Emission from 3K Background Photons

D. E. Harris, L. S. Moore

astro-pharXiv:astro-ph/0002463

Abstract

We review the history and a few features of IC/3K emission. We discuss observing strategies, the physical parameters which can be derived directly or indirectly from successful detections, and the disparities between magnetic field strength estimates found by different methods.

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