Open AccessA spectropolarimetric atlas of Seyfert 1 galaxies
Author(s) -
Smith J. E.,
Young S.,
Robinson A.,
Corbett E. A.,
Giannuzzo M. E.,
Axon D. J.,
Hough J. H.
Publication year - 2002
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.2002.05665.x
Subject(s) - physics , galaxy , astrophysics , polarization (electrochemistry) , astronomy , position angle , active galactic nucleus , line of sight , luminous infrared galaxy , polar , scattering , radio galaxy , emission spectrum , spectral line , optics , chemistry
We present optical spectropolarimetry of the nuclei of 36 Seyfert 1 galaxies, obtained with the William Herschel and the Anglo‐Australian Telescopes from 1996 to 1999. In 20 of these, the optical emission from the active nucleus is intrinsically polarized. We have measured a significant level of polarization in a further seven objects but these may be heavily contaminated by Galactic interstellar polarization. The intrinsically polarized Seyfert 1 galaxies exhibit a variety of characteristics, with the average polarization ranging from <0.5 to 5 per cent and with many showing variations in both the degree and position angle of polarization across the broad Hα emission line. We identify a small group of Seyfert 1 galaxies that exhibit polarization properties similar to those of Seyfert 2 galaxies in which polarized broad lines have been discovered. These objects represent direct observational evidence that a Seyfert 2‐like far‐field polar scattering region is also present in Seyfert 1 galaxies. Several other objects have features that can be explained in terms of equatorial scattering of line emission from a rotating disc. We propose that much of the diversity in the polarization properties of Seyfert galaxies can be understood in terms of a model involving both equatorial and polar scattering, the relative importance of the two geometries as sources of polarized light being determined principally by the inclination of the system axis to the line of sight.