Investigating the central engine of Seyfert 2 galaxies with and without Polarized Broad Lines

Abstract

We study the hard X-ray emission of two samples of Seyfert 2 galaxies with and without Polarized Broad Lines (PBL). In the hard X-ray domain, absorption effects do not significantly modify the intrinsic emission allowing us a direct access to the central engine. The purpose of this study is to compare the primary emission of the two Seyfert 2 subclasses in order to investigate the nature of their central engine and to test unified models according to which they both have a hidden Seyfert 1 nucleus. We compute the average hard X-ray spectra of Seyfert 2 galaxies with and without PBL observed with BeppoSAX/PDS (15-136 keV). The two spectra have a common general behavior at first sight, but investigating deeper we find differences in the intrinsic properties of the two categories of Seyfert 2 galaxies. Sy 2 with polarized broad lines have physical conditions close to those of Sy 1 galaxies whereas Sy 2 without PBL differ substantially, suggesting that they may have a particular place in the scheme of Seyfert galaxies.

10 pages, accepted for publication in A&A

References in corpus (2)

• The Unified Model & Evolution of Active Galaxies: Implications from a Spectropolarimetric Study
• The intrinsic emission of Seyfert galaxies observed with BeppoSAX/PDS I. Comparison of the average spectra of the three classes of Seyfert Galaxies

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• Narrow Line Seyfert 1 galaxies at hard X-rays
• The Unified Model of Active Galactic Nuclei: I. Non-hidden Broad Line Region Seyfert 2 and Narrow Line Seyfert 1 Galaxies
• INTEGRAL observations of AGN in the Galactic Plane
• The study of Seyfert 2 galaxies with and without infrared broad lines
• Ionization Mechanisms of HBLR and Non-HBLR Seyfert 2 Galaxies