Hidden broad line regions and anisotropy in AGN

Details Hidden broad line regions and anisotropy in AGN Hidden broad line regions and anisotropy in AGN

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..379a&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 379-398

Astronomy and Astrophysics

Astronomy

8

Active Galactic Nuclei, Anisotropy, Astronomical Polarimetry, Grand Unified Theory, Infrared Astronomy, Radio Galaxies, Seyfert Galaxies, Astronomical Maps, Astronomical Spectroscopy, H Alpha Line, Infrared Spectroscopy, Signal To Noise Ratios, Stellar Luminosity

Scientific paper

We discuss the recent advances made in the search for hidden broad line regions in Seyfert and Narrow Line Radio Galaxies (NLRG) using both spectropolarimetry and infrared spectroscopy/spectropolarimetry. Two important results which support the Grand Unification Theory are presented. In the first of these we report that the famous Seyfert 1 NGC 4151 has a scattered component to its broad line region, and is most likely an object where we view obliquely into its occulting torus. In the second, we show high signal to noise observations of scattered broad lines in the NRLG of 3C 234.

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