Emission and Absorption Properties of Low-Mass Type 2 Active Galaxies with XMM-Newton
arXiv:0910.1603 · doi:10.1088/0004-637X/705/2/1196
Abstract
We present XMM-Newton observations of four low-redshift Seyfert galaxies selected to have low host luminosities (M_g>-20 mag) and small stellar velocity dispersions (sigma_star<45 km/s), which are among the smallest stellar velocity dispersions found in any active galaxies. These galaxies show weak or no broad optical emission lines and have likely black hole masses <10^6 M_sun. Three out of four objects were detected with >3sigma significance in ~25 ks exposures and two observations had high enough signal-to-noise ratios for rudimentary spectral analysis. We calculate hardness ratios (-0.43 to 0.01) for the three detected objects and use them to estimate photon indices in the range of Gamma=1.1-1.8. Relative to [OIII], the type 2 objects are X-ray faint in comparison with Seyfert 1 galaxies, suggesting that the central engines are obscured. We estimate the intrinsic absorption of each object under the assumption that the [OIII] emission line luminosities are correlated with the unabsorbed X-ray luminosity. The results are consistent with moderate (N_H~10^22 cm^-2) absorption over the Galactic values in three of the four objects, which might explain the non-detection of broad-line emission in optical spectra. One object in our sample, SDSS J110912.40+612346.7, is a near identical type 2 counterpart of the late-type Seyfert 1 galaxy NGC 4395. While the two objects have very similar [OIII] luminosities, the type 2 object has an X-ray/[OIII] flux ratio nearly an order of magnitude lower than NGC 4395. The most plausible explanation for this difference is absorption of the primary X-ray continuum of the type 2 object, providing an indication that obscuration-based unified models of active galaxies can apply even at the lowest luminosities seen among Seyfert nuclei, down to L_bol~10^40-10^41 erg/s.
5 figures, 3 tables, accepted for publication in ApJ
References in corpus (22)
- The Host Galaxies and Classification of Active Galactic Nuclei
- Piecing Together the X-ray Background: Bolometric Corrections for Active Galactic Nuclei
- X-ray spectral properties of AGN in the Chandra Deep Field South
- A New Sample of Low-mass Black Holes in Active Galaxies
- Simultaneous X-ray/optical/UV snapshots of active galactic nuclei from XMM-Newton: spectral energy distributions for the reverberation mapped sample
- On the X-ray, optical emission line and black hole mass properties of local Seyfert galaxies
- The Coincidence of Nuclear Star Clusters and Active Galactic Nuclei
- The bolometric luminosity of type 2 AGN from extinction-corrected [OIII]: no evidence for Eddington-limited sources
- Spitzer Uncovers Active Galactic Nuclei Missed by Optical Surveys in 7 Late-type Galaxies
- AMUSE-Virgo I. Super-massive black holes in low-mass spheroids
- The Correlation of Narrow Line Emission and X-ray Luminosity in Active Galactic Nuclei
- The Host Galaxy and Central Engine of the Dwarf AGN POX 52
- X-ray Properties of Intermediate-mass Black Holes in Active Galaxies
- The XMM-Newton view of AGN with intermediate mass black holes
- Tracing the Mass-Dependent Star Formation History of Late-Type Galaxies using X-ray Emission: Results from the Chandra Deep Fields
- Low-Mass Seyfert 2 Galaxies in the Sloan Digital Sky Survey
- X-ray Properties of Intermediate-Mass Black Holes in Active Galaxies. II. X-ray-Bright Accretion and Possible Evidence for Slim Disks
- On the nature of unabsorbed Seyfert 2 galaxies
- NGC3147: a "true" Seyfert 2 without the broad-line region
- Chandra Observations of Candidate "True" Seyfert 2 Nuclei
- 4U 1344-60: a bright intermediate Seyfert galaxy at z=0.012 with a relativistic Fe Kalpha emission line
- Detection of blueshifted emission and absorption and a relativistic Iron line in the X-ray spectrum of ESO 323-G077
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- Coevolution (Or Not) of Supermassive Black Holes and Host Galaxies
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- X-ray Properties of Intermediate-mass Black Holes in Active Galaxies. III. Spectral Energy Distribution and Possible Evidence for Intrinsically X-ray-weak AGNs
- The Low-mass, Highly Accreting Black Hole Associated with the Active Galactic Nucleus 2XMM J123103.2+110648
- X-ray Spectral and Variability Properties of Low-Mass AGN
- Chandra and MMT observations of low-mass black hole active galactic nuclei accreting at low rates in dwarf galaxies
- Is IRAS 01072+4954 a True-Seyfert 2? Hints from Near Infrared Integral Field Spectroscopy
- Low-Mass Active Galactic Nuclei with Rapid X-Ray Variability
- A Comprehensive Archival Chandra Search for X-ray Emission from Ultracompact Dwarf Galaxies
- A New Sample of Obscured AGNs Selected from the XMM-Newton and AKARI Surveys
- NuSTAR observations of a heavily X-ray obscured AGN in the dwarf galaxy J144013+024744