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Distribution of synchrotron relativistic plasma emission over quasar radio lobes

Distribution of synchrotron relativistic plasma emission over quasar radio lobes

Asymmetrical lobe structures of radio galaxies and quasars can be explained in the diffusion model with the moving hot spot (the source of ultra relativistic electron plasma) by the possible jet precession. The equation for the space-time nonuniform electron distribution function, describing the syn...

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Bibliographic Details
Main Authors: Kontorovich, V.M., Kolesnikov, F.M.
Format: Article
Language:English
Published: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2001
Series:Вопросы атомной науки и техники
Subjects:
Electrodynamics of high energies in matter and strong fields
Online Access:http://dspace.nbuv.gov.ua/handle/123456789/79479
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http://dspace.nbuv.gov.ua/handle/123456789/79479

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