The wavelength dependence of polarization in active galactic nuclei

Details The wavelength dependence of polarization in active galactic nuclei The wavelength dependence of polarization in active galactic nuclei

2003-04-14

arxiv.org/abs/astro-ph/0304243v2

Astronomy and Astrophysics

Astrophysics

4 pages, LaTeX

Scientific paper

Using 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.

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