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
Published in:Вопросы атомной науки и техники
Date:2001
Main Authors: Kontorovich, V.M., Kolesnikov, F.M.
Format: Article
Language:English
Published: Національний науковий центр «Харківський фізико-технічний інститут» НАН України 2001
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79479
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Distribution of synchrotron relativistic plasma emission over quasar radio lobes / V.M. Kontorovich, F.M. Kolesnikov // Вопросы атомной науки и техники. — 2001. — № 6. — С. 171-175. — Бібліогр.: 15 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine