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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| Published in: | Вопросы атомной науки и техники |
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| Date: | 2001 |
| Main Authors: | , |
| Format: | Article |
| Language: | English |
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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| id |
nasplib_isofts_kiev_ua-123456789-79479 |
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Kontorovich, V.M. Kolesnikov, F.M. 2015-04-02T15:25:37Z 2015-04-02T15:25:37Z 2001 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. 1562-6016 PACS: 98.54.G https://nasplib.isofts.kiev.ua/handle/123456789/79479 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 synchrotron losses and the diffusion of electrons from the hot spot into the lobes, is solved analytically. The space distributions of the synchrotron emission intensity and the spectral indices on the lobe are calculated numerically for different parameters of the jet precession and the diffusion. en Національний науковий центр «Харківський фізико-технічний інститут» НАН України Вопросы атомной науки и техники Electrodynamics of high energies in matter and strong fields Distribution of synchrotron relativistic plasma emission over quasar radio lobes Распределение излучения синхротронной релятивистской плазмы по протяженным компонентам радио квазаров Article published earlier |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Distribution of synchrotron relativistic plasma emission over quasar radio lobes |
| spellingShingle |
Distribution of synchrotron relativistic plasma emission over quasar radio lobes Kontorovich, V.M. Kolesnikov, F.M. Electrodynamics of high energies in matter and strong fields |
| title_short |
Distribution of synchrotron relativistic plasma emission over quasar radio lobes |
| title_full |
Distribution of synchrotron relativistic plasma emission over quasar radio lobes |
| title_fullStr |
Distribution of synchrotron relativistic plasma emission over quasar radio lobes |
| title_full_unstemmed |
Distribution of synchrotron relativistic plasma emission over quasar radio lobes |
| title_sort |
distribution of synchrotron relativistic plasma emission over quasar radio lobes |
| author |
Kontorovich, V.M. Kolesnikov, F.M. |
| author_facet |
Kontorovich, V.M. Kolesnikov, F.M. |
| topic |
Electrodynamics of high energies in matter and strong fields |
| topic_facet |
Electrodynamics of high energies in matter and strong fields |
| publishDate |
2001 |
| language |
English |
| container_title |
Вопросы атомной науки и техники |
| publisher |
Національний науковий центр «Харківський фізико-технічний інститут» НАН України |
| format |
Article |
| title_alt |
Распределение излучения синхротронной релятивистской плазмы по протяженным компонентам радио квазаров |
| description |
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 synchrotron losses and the diffusion of electrons from the hot spot into the lobes, is solved analytically. The space distributions of the synchrotron emission intensity and the spectral indices on the lobe are calculated numerically for different parameters of the jet precession and the diffusion.
|
| issn |
1562-6016 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/79479 |
| citation_txt |
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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| first_indexed |
2025-12-07T20:57:08Z |
| last_indexed |
2025-12-07T20:57:08Z |
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