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Modeling the Polarization of Dusty Scattering Cones in Active Galactic Nuclei

Rene W. Goosmann·C. Martin Gaskell·M. Shoji
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Abstract

We have used the STOKES radiative transfer code, to model polarization induced by dust scattering in the polar regions of Active Galactic Nuclei (AGN). We discuss the wavelength-dependence of the spectral intensity and polarization over the optical/UV range at different viewing angles for two different types of dust: a Galactic dust model, and a dust model inferred from extinction properties of AGN. The STOKES code and documentation are freely available at http://www.stokes-program.info/.

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Rene W. Goosmann, C. Martin Gaskell, M. Shoji. 2007-01-07. Modeling the Polarization of Dusty Scattering Cones in Active Galactic Nuclei. https://arxiv.org/abs/astro-ph/0701163

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