The wavelength dependence of polarization in active galactic nuclei

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dc.creatorPrigara, F. V.
dc.date2003-04-14
dc.date2003-11-12
dc.date.accessioned2026-07-25T11:57:47Z
dc.descriptionUsing the gaseous disk model and the condition for emission based on a stimulated origin of thermal radio emission (Prigara 2003), we received the wavelength dependence of polarization for radio emission from active galactic nuclei consistent with available observational data. The strength of magnetic field required to produce an observable degree of polarization in active galactic nuclei is discussed.
dc.description4 pages, LaTeX
dc.identifierhttps://arxiv.org/abs/astro-ph/0304243
dc.identifierhttp://arxiv.org/abs/astro-ph/0304243
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/6831
dc.subjectAstrophysics
dc.titleThe wavelength dependence of polarization in active galactic nuclei
dc.typetext

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