An optical and near-infrared polarization survey of Seyfert and broad-line radio galaxies. 1 : statistical properties
Brindle, C.; Hough, J.; Bailey, J.; Axon, D.J.; Ward, M.J.; Sparks, W.; McLean, I.
Citation: Brindle , C , Hough , J , Bailey , J , Axon , D J , Ward , M J , Sparks , W & McLean , I 1990 , ' An optical and near-infrared polarization survey of Seyfert and broad-line radio galaxies. 1 : statistical properties ' Monthly Notices of the Royal Astronomical Society , vol 244 , no. 4 , pp. 577-603 .
The present broad-band and near-IR flux density and polarization measurements of a sample of 71 Seyfert galaxies and three broad-line radio galaxies confirms earlier indications that the polarization of Seyferts is generally low in the V-band and at longer wavelengths. A tendency is noted for the polarization to be parallel to the galaxy optical or dust-lane axis; previous indications that the polarization of Seyfert 2s tends to be perpendicular to the radio axis are confirmed. In the second part of this work, the 0.44-2.2 micron wavelength dependence of polarization for this sample of 71 Seyfert and three broad-line radio galaxies is discussed. Most objects in the sample exhibit decreasing polarization with increasing wavelength, as may be expected in polarization induced by either dichroic absorption or scattering.
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