Conical accretion disc models using the Milne problem predict reduced polarization and opposite position angles from ring segments, providing a geometric account for spectral line wing polarization in Seyfert galaxies.
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Radiation intensity and polarization from accretion discs with progressive increasing height
Conical accretion disc models using the Milne problem predict reduced polarization and opposite position angles from ring segments, providing a geometric account for spectral line wing polarization in Seyfert galaxies.