Some Aspects of Inverse Compton Emission from 3K Background Photons

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dc.creatorHarris, D. E.
dc.creatorMoore, L. S.
dc.date2000-02-24
dc.date.accessioned2026-07-07T01:52:29Z
dc.date.available2026-07-07T01:52:29Z
dc.descriptionWe 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.
dc.description4 pages latex with one embedded figure.Published in MPE Report 271, October 1999, page 219. Proceedings of the Ringberg workshop: "Diffuse Thermal and Relativistic Plasma in Galaxy Clusters", editors H. Böhringer, L. Feretti, and P. Schuecker
dc.identifierhttps://arxiv.org/abs/astro-ph/0002463
dc.identifierhttp://arxiv.org/abs/astro-ph/0002463
dc.identifierMPE Report 271, October 1999, page 219
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/635
dc.subjectAstrophysics
dc.titleSome Aspects of Inverse Compton Emission from 3K Background Photons
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