University of Hertfordshire

From the same journal

From the same journal

By the same authors

  • C. Brindle
  • J. Hough
  • J. Bailey
  • D.J. Axon
  • M.J. Ward
  • W. Sparks
  • I. McLean
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Original languageEnglish
Pages (from-to)577-603
JournalMonthly Notices of the Royal Astronomical Society
Journal publication date1990
Volume244
Issue4
Publication statusPublished - 1990

Abstract

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.

Notes

Copyright Royal Astronomical Society. [Full text of this article is not available in the UHRA]

ID: 153167