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• W3104229951 startingPage "A66" @default.
• W3104229951 abstract "Context. A growing body of evidence suggests that some, if not all, scattering regions of active galactic nuclei (AGNs) are clumpy. The inner AGN components cannot be spatially resolved with current instruments and must be studied by numerical simulations of observed spectroscopy and polarization data." @default.
• W3104229951 created "2020-11-23" @default.
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• W3104229951 date "2015-05-01" @default.
• W3104229951 modified "2023-10-14" @default.
• W3104229951 title "Modeling optical and UV polarization of AGNs" @default.
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• W3104229951 doi "https://doi.org/10.1051/0004-6361/201525628" @default.
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