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Related papers: Hidden Broad-line Regions in Seyfert 2 Galaxies: f…

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According to the unified model of active galactic nuclei, Seyfert 2 galaxies are physically the same as Seyfert 1 objects and they possess a broad-line region (BLR), but it is hidden from the observer due to their orientation. In the past…

Astrophysics of Galaxies · Physics 2016-11-17 Georgi P. Petrov

The unified model of Seyfert galaxies suggests that there are hidden broad-line regions (HBLRs) in Seyfert 2 galaxies (S2s). However, there is increasing evidence for the appearance of a subclass of S2s lacking of HBLR (non-HBLR S2s). An…

Astrophysics · Physics 2008-11-26 E. -P Zhang , J. -M. Wang

We compile a large sample of 120 Seyfert 2 galaxies (Sy2s) which contains 49 hidden broad-line region (HBLR) Sy2s and 71 non-HBLR Sy2s. From the difference in the power sources between two groups, we test if HBLR Sy2s are dominated by…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Yu-Zhong Wu , En-Peng Zhang , Yan-Chun Liang , Cheng-Min Zhang , Yong-Heng Zhao

We extend the analysis presented in Tran (2001) of a spectropolarimetric survey of the CfA and 12micron samples of Seyfert 2 galaxies (S2s). We confirm that S2s with hidden broad line regions (HBLRs) tend to have hotter circumnuclear dust…

Astrophysics · Physics 2009-11-07 Hien D. Tran

We report the results of a spectropolarimetric survey of the CfA and 12micron samples of Seyfert 2 galaxies (S2s). Polarized (hidden) broad line regions (HBLRs) are confirmed in a number of galaxies, and several new cases (F02581-1136, MCG…

Astrophysics · Physics 2009-11-06 Hien D. Tran

The evidence is reviewed that the Broad Line Region (BLR) probably has two distinct components located at about the same distance from the central black hole. One component, BLR II, is optically-thick, low-ionization emission at least some…

Astrophysics · Physics 2009-10-31 C. Martin Gaskell

High angular resolution spectroscopy obtained with the Hubble Space Telescope (HST) has revealed a remarkable population of galaxies hosting dwarf Seyfert nuclei with an unusually large broad-line region (BLR). These objects are remarkable…

Astrophysics of Galaxies · Physics 2016-01-20 Nick Devereux

We study the disk emission component hidden in the single-peaked Broad Emission Lines (BELs) of Active Galactic Nuclei (AGN). We compare the observed broad lines from a sample of 90 Seyfert 1 spectra taken from the Sloan Digital Sky Survey…

Astrophysics of Galaxies · Physics 2015-05-14 E. Bon , L. Č. Popović , N. Gavrilović , G. La Mura , E. Mediavilla

We report the discovery of the scattered emission from a hidden broad-line region (BLR) in a Seyfert 2 galaxy, Mrk 573, based on our recent spectropolarimetric observation performed at the Subaru Telescope. This object has been regarded as…

The Broad Emission Lines (BELs) in spectra of type 1 Active Galactic Nuclei (AGN) can be very complex, indicating a complex Broad Line Region (BLR) geometry. According to the standard unification model one can expect an accretion disk…

High Energy Astrophysical Phenomena · Physics 2014-11-20 E. Bon , N. Gavrilovic , G. La Mura , L. C. Popovic

In this paper I present evidence suggesting that the absence or presence of Hidden Broad Line Regions (HBLRs) in Seyfert 2 galaxies is regulated by the rate at which matter accretes onto a central supermassive black hole, in units of…

Astrophysics · Physics 2007-05-23 F. Nicastro , A. Martocchia , G. Matt

The results of spectropolarimetry surveys of obscured AGNs are reviewed, paying special attention to their implications for the existence of two populations of type 2 Seyfert galaxies -- hidden Seyfert 1s and "true" Seyfert 2s. In this…

Astrophysics · Physics 2007-05-23 Edward C. Moran

In the past few years more and more pieces of evidence have been presented for a revision of the widely accepted Unified Model of Active Galactic Nuclei. A model based solely on orientation cannot explain all the observed phenomenology. In…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 Andrea Marinucci , Stefano Bianchi , Fabrizio Nicastro , Giorgio Matt , Andy D. Goulding

Using a large sample of 90 Seyfert 2 galaxies (Sy2s) with spectropolarimetric observations, we tested the suggestion that the presence of hidden broad-line regions (HBLRs) in Sy2s is dependent upon the Eddington ratio. The stellar velocity…

Astrophysics · Physics 2008-11-26 W. Bian , Q. Gu

In this paper we present evidence suggesting that the absence or presence of Hidden Broad Line Regions (HBLRs) in Seyfert 2 galaxies is regulated by the rate at which matter accretes onto a central supermassive black hole, in units of…

Astrophysics · Physics 2009-11-07 F. Nicastro , A. Martocchia , G. Matt

We present a compilation of radio, infrared, optical and hard X-ray (2-10kev) data for a sample of 90 Seyfert 2 galaxies(Sy2s) with spectropolarimetric observations (41 Sy2s with detection of polarized broad lines (PBL) and 49 without PBL).…

Astrophysics · Physics 2016-08-17 Qiusheng Gu Jiehao Huang

Based on the analysis of a large spectropolarimetric survey of Seyfert 2 galaxies (S2s) from the CfA and 12-micron samples conducted mostly at Lick and Palomar Observatories, it is shown that S2s with hidden BLR (HBLRs) are intrinsically…

Astrophysics · Physics 2007-05-23 Hien D. Tran

We analyze the properties of the broad line region (BLR) in low luminosity AGN by using HST/STIS spectra. We consider a sample of 24 nearby galaxies in which the presence of a BLR has been reported from their Palomar ground-based spectra.…

Astrophysics of Galaxies · Physics 2015-06-18 B. Balmaverde , A. Capetti , INAF - Osservatorio Astrofisico di Torino

I review progress made in understanding the nature of the broad-line region (BLR) of active galactic nuclei (AGNs) and the role BLRs play in the AGN phenomenon. The high equivalent widths of the lines imply a high BLR covering factor, and…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-13 C. Martin Gaskell

We present the results of the long-term optical monitoring campaign of active galactic nuclei (AGN) coordinated by the Special Astrophysical Observatory of the Russian Academy of Science. This campaign has produced a remarkable set of…

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