The distribution of absorbing column densities among Seyfert 2 galaxies
arXiv:astro-ph/9902377 · doi:10.1086/307623
Abstract
We use hard X-ray data for an "optimal" sample of Seyfert 2 galaxies to derive the distribution of the gaseous absorbing column densities among obscured active nuclei in the local Universe. Of all Seyfert 2 galaxies in the sample, 75% are heavily obscured (N_H > 10^23 cm^-2) and about half are Compton thick (N_H > 10^24 cm^-2). Intermediate type 1.8-1.9 Seyferts are characterized by an average N_H much lower than "strict" Seyfert 2s. No correlation is found between N_H and the intrinsic luminosity of the nuclear source. This N_H distribution has important consequences for the synthesis of the cosmic X-ray background. Also, the large fraction of Compton thick objects implies that most of the obscuring gas is located within a radius of a few 10 pc from the nucleus.
arXiv comment16 LaTeX pages+5 postscript figures, accepted by ApJ
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- Hidden AGNs in Early-Type Galaxies
- Unsupervised Machine Learning for the Classification of Astrophysical X-ray Sources
- ALMA observations of the submillimetre hydrogen recombination line from the type 2 active nucleus of NGC 1068
- A Model for Type 2 Coronal Line Forest (CLiF) AGN
- Clumpy winds and the obscuration of Active Galactic Nuclei
- Chandra Reveals Heavy Obscuration and Circumnuclear Star Formation in Seyfert 2 Galaxy NGC 4968
- A unique X-ray unabsorbed Seyfert 2 galaxy IRAS F01475-0740
- Evolution of luminosity function and obscuration of AGN: connecting X-ray and Infrared
- Rolling down from the 30 keV peak: modelling the hard X-ray and gamma-ray backgrounds
- Comparing Chandra and SIRTF Observations for Obscured Starbursts and AGN at High Redshift
- On the Evolution of High-Redshift Active Galactic Nuclei
- X-ray Spectroscopy and Variability of AGN Detected in the 2 Ms Chandra Deep Field-North Survey
- The interaction of the active nucleus with the host galaxy interstellar medium
- Isolated AGNs NGC 5347, ESO 438-009, MCG-02-04-090, and J11366-6002: Swift and NuSTAR joined view
- XMM Observations of the Seyfert 2 Galaxy NGC 7590: the Nature of X-ray Absorption
- XMM Follow-Up Observations of Three Swift BAT-Selected Active Galactic Nuclei
- Suzaku X-ray spectral study of the Compton-thick Seyfert galaxy NGC 5135
- Characterization of AGN and their hosts in the Extended Groth Strip: a multiwavelength analysis
- AGN Triality of Triple Mergers: Multi-wavelength Classifications
- Are Seyfert 2 Galaxies without Polarized Broad Emission Lines More Obscured?
- MIRACLE I.: Unveiling the Multi-Phase, Multi-Scale physical properties of the Active Galaxy NGC 424 with MIRI, MUSE, and ALMA
- A candidate Optically Quiescent Quasar lacking narrow emission lines
- The study of Seyfert 2 galaxies with and without infrared broad lines
- The XMM spectral catalog of SDSS optically selected Seyfert 2 galaxies
- Probing the roles of orientation and multi-scale gas distributions in shaping the obscuration of Active Galactic Nuclei through cosmic time
- The Young, the Old, and the Dusty: Stellar Populations of AGN Hosts
- Evolution of supermassive black holes
- Classical radio source propagating into outer HI disc in NGC 3801
- The Awakening Beast in the Seyfert 1 Galaxy KUG 1141+371 I
- On the fate of the matter reinserted within young nuclear stellar clusters
- Analysis of the Interaction Effects in the Southern Galaxy Pair Tol1238-364 and ESO381-G009
- Inferring Compton-thick AGN candidates at z>2 with Chandra using the >8 keV restframe spectral curvature
- X-ray Eclipses of Active Galactic Nuclei
- Detecting quasars at very high redshift with next generation X-ray telescopes
- X-ray Survey Results on Active Galaxy Physics and Evolution
- Searching for obscured AGN in z 2 submillimetre galaxies
- The luminous infrared composite Seyfert 2 galaxy NGC 7679 through the [O III] 5007 emission line
- A Statistical Study of H I Gas in Nearby Narrow-Line AGN-Hosting Galaxies
- X-ray view of four high-luminosity Swift/BAT AGN: Unveiling obscuration and reflection with Suzaku
- Distant X-ray Galaxies: Insights from the Local Population
- The hard X-ray view of bright infrared galaxies
- Active Galactic Nuclei and their demography through cosmic time
- Multiwavelength Analysis of a Nearby Heavily Obscured AGN in NGC 449
- XMMU J134736.6+173403: an eclipsing LMXB in quiescence or a peculiar AGN?
- X-ray selection of Compton Thick AGN at high redshift
- VLBI Detection of an Active Radio Source Potentially Driving 100-kpc Scale Emission in the Ultraluminous Infrared Galaxy IRAS F010042237
- An excess of low-mass X-ray binaries in the outer halo of NGC 4472
- The X-ray Nature of Nucleus in Seyfert 2 Galaxy NGC 7590
- Characterisation of AGN from the XMM-Newton Slew Survey
- The XMM-SSC survey of hard-spectrum XMM-Newton sources 1: optically bright sources
- A new panchromatic classification of unclassified Burst Alert Telescope active galactic nuclei
- On the origin of the X-ray emission from a narrow-line radioquasar at z>1
- Supermassive Black Holes in Deep Multiwavelength Surveys
- Aspects of astrophysical particle production and beyond the Standard Model phenomenology
- The Distribution of Hard X-ray Selected AGN in the NEP Field
- The XMM-Newton hard band wide angle Survey
- MIDIS: Quantifying the AGN component of X-ray-detected galaxies
- A multiwavelength study of near- and mid-infrared selected galaxies at high redshift: ERGs, AGN-identification and the contribution from dust
- X-ray properties of two complementary samples of intermediate Seyfert galaxies
- Optical Variability Structure Function of Low-Luminosity AGN using ATLAS Lightcurves
- Chandra Follow-up Observations of Swift-BAT-selected AGNs II