On the nature of Seyfert galaxies with high [OIII]5007 blueshifts
arXiv:0803.0240 · doi:10.1086/587932
Abstract
We have studied the properties of Seyfert galaxies with high [OIII]5007 blueshifts (`blue outliers'), originally identified because of their strong deviation from the M_BH - sigma relation of normal, narrow-line Seyfert 1 (NLS1) and broad-line Seyfert 1 (BLS1) galaxies. These blue outliers turn out to be important test-beds for models of the narrow-line region (NLR), for mechanisms of driving large-scale outflows, for links between NLS1 galaxies and radio galaxies, and for orientation-dependent NLS1 models. We report the detection of a strong correlation of line blueshift with ionization potential in each galaxy, including the measurement of coronal lines with radial velocities up to 500--1000 km/s. All [OIII] blue outliers have narrow widths of their broad Balmer lines and high Eddington ratios. While the presence of non-shifted low-ionization lines signifies the presence of a classical outer quiescent NLR in blue outliers, we also report the absence of any second, non-blueshifted [OIII] component from a classical inner NLR. These results place tight constraints on NLR models. We favor a scenario in which the NLR clouds are entrained in a decelerating wind which explains the strong stratification and the absence of a zero-blueshift inner NLR of blue outliers. The origin of the wind remains speculative at this time (collimated radio plasma, thermal winds, radiatively accelerated clouds). It is perhaps linked to the high Eddington ratios of blue outliers. Similar, less powerful winds could be present in all Seyfert galaxies, but would generally only affect the coronal line region (CLR), or level off even before reaching the CLR. Similarities between blue outliers in NLS1 galaxies and (compact) radio sources are briefly discussed.
ApJ in press (scheduled for June 20 issue); incl. 4 colour figures. This, and related paper showing that NLS1 galaxies follow the M-sigma relation based on [SII], is also available at http://www.xray.mpe.mpg.de/~skomossa/
References in corpus (22)
- A Comprehensive Study of 2 000 Narrow Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey: I. The Sample
- Radio-loud Narrow-Line Type 1 Quasars
- CIV 1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei
- A Survey of Kiloparsec-Scale Radio Outflows in Radio-Quiet Active Galactic Nuclei
- Cosmic Evolution of Mass Accretion Rate and Metalicity in Active Galactic Nuclei
- Size and properties of the narrow-line region in Seyfert-1 galaxies from spatially-resolved optical spectroscopy
- Narrow-line Seyfert 1 Galaxies and the M_BH - sigma Relation
- The co-evolution of the obscured quasar PKS1549-79 and its host galaxy: evidence for a high accretion rate and warm outflow
- Radiative pressure feedback by a quasar in a galactic bulge
- Outflows of very ionized gas in the center of Seyfert galaxies: kinematics and physical conditions
- IC5063: AGN driven outflow of warm and cold gas
- Dynamics of Rotating Accretion Flows Irradiated by a Quasar
- Gemini Near Infrared Integral Field Spectroscopy of the Narrow-Line Region of ESO428-G14: kinematics, excitation and the role of the radio jet
- Dynamics of the Narrow-Line Region in the Seyfert 2 Galaxy NGC 1068
- The Central Engines of Narrow-Line Seyfert 1 Galaxies
- Simulations of Metal Enrichment in Galaxy Clusters by AGN Outflows
- The narrow-line region of narrow-line and broad-line type 1 AGN I. A zone of avoidance in density
- Large-Scale Parker Winds in Active Galactic Nuclei
- Entrainment Mechanisms for Outflows in the L1551 Star-Forming Region
- A Balmer-line Broad Absorption Line Quasar
- Revisiting the Black Hole Masses of Soft X-ray-Selected Active Galactic Nuclei
- Simulations of the interaction of cold gas with radio jets
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- A Population of Radio-loud Narrow Line Seyfert 1 Galaxies with Blazar-like Properties?
- VLT/ISAAC Spectra of the Hbeta Region in Intermediate-Redshift Quasars III. Hbeta Broad Line Profile Analysis and Inferences about BLR Structure
- Very Broad [O III]4959,5007 Emission from the NGC 4472 Globular Cluster RZ2109 and Implications for the Mass of Its Black Hole X-ray Source
- The Narrow-Line Region of Narrow-Line Seyfert 1 Galaxies