Broad Line Region Physical Conditions along the Quasar Eigenvector 1 Sequence
arXiv:1007.3187 · doi:10.1111/j.1365-2966.2010.17357.x
Abstract
[Abridged] We compare broad emission line profiles and estimate line ratios for all major emission lines between Ly-alpha and H-beta in a sample of six quasars. The sources were chosen with two criteria in mind: the existence of high quality optical and UV spectra as well as the possibility to sample the spectroscopic diversity in the 4D Eigenvector 1 context . In the latter sense each source occupies a region (bin) in the FWHM(H-beta) vs. optical FeII strength plane that is significantly different from the others. High S/N H-beta emission line profiles are used as templates for modeling the other lines (Ly-alpha, CIV 1549, HeII 1640, Al III 1860, Si III] 1892, and Mg II 2800). We can adequately model all broad lines assuming the existence of three components distinguished by blueshifted, unshifted and redshifted centroids (indicated as blue, broad and very broad component respectively). The broad component (high electron density, low ionization parameter; high column density) is present in almost all type-1 quasars and therefore corresponds most closely to the classical broad line emitting region (the reverberating component). The blue component emission (lower electron density; high ionization; low column density) arises in less optically thick gas; it is often thought to arise in an accretion disk wind. The least understood component involves the very broad component (high ionization and large column density). It is perhaps the most distinguishing characteristic of quasars with FWHM H-beta > 4000 km/s that belong to the so-called Population B of our 4DE1 space. Population A quasars (FWHM H-beta < 4000 km/s) are dominated by broad component emission in H-beta and blue component emission in CIV 1549 and other high ionization lines. 4DE1 appears to be the most useful current context for revealing and unifying spectral diversity in type-1 quasars.
7 Tables, 5 Figures; accepted for publication in Monthly Notices of the Royal Astronomical Society
References in corpus (43)
- Composite Quasar Spectra From the Sloan Digital Sky Survey
- Central Masses and Broad-Line Region Sizes of Active Galactic Nuclei. II. A Homogeneous Analysis of a Large Reverberation-Mapping Database
- Determining Central Black Hole Masses in Distant Active Galaxies and Quasars. II. Improved Optical and UV Scaling Relationships
- An Empirical Ultraviolet Template for Iron Emission in Quasars as Derived from I Zw 1
- Broad Emission Line Shifts in Quasars: An Orientation Measure for Radio-Quiet Quasars?
- The effect of radiation pressure on virial black hole mass estimates and the case of Narrow Line Seyfert 1 galaxies
- Completion of a Survey and Detailed Study of Double-Peaked Emission Lines in Radio-Loud AGNs
- CIV 1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei
- Double-Peaked Low-Ionization Emission Lines in Active Galactic Nuclei
- What the Optical Recombination Lines Can Tell Us About the Broad Line Regions of Active Galactic Nuclei
- Estimating Black Hole Masses in Active Galactic Nuclei Using the MgII 2800 Emission Line
- Near Infrared Spectroscopy of High Redshift Active Galactic Nuclei. I. A Metallicity-Accretion Rate Relationship
- Star Formation Around Super-Massive Black Holes
- Searching for the Physical Drivers of the Eigenvector 1 Correlation Space
- Diverse Broad Line Region Kinematic Signatures From Reverberation Mapping
- Average Quasar Spectra in the Context of Eigenvector 1
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- The metallicity of the most distant quasars
- Detailed Characterization of H_beta emission line profile in low z SDSS quasars
- Searching For the Physical Drivers of Eigenvector 1: Influence of Black Hole Mass and Eddington Ratio
- Average UV Quasar Spectra in the Context of Eigenvector 1: A Baldwin Effect Governed by Eddington Ratio?
- Long-Term Profile Variability of Double Peaked Emission Lines in Active Galactic Nuclei
- VLT/ISAAC Spectra of the Hbeta Region in Intermediate-Redshift Quasars III. Hbeta Broad Line Profile Analysis and Inferences about BLR Structure
- New Insights on the QSO Radio-Loud/Radio-Quiet Dichotomy: SDSS Spectra in the Context of the 4D Eigenvector1 Parameter Space
- Implications of infalling Fe II - emitting clouds in active galactic nuclei: anisotropic properties
- Long-term variability of the optical spectra of NGC 4151: II. Evolution of the broad Ha and Hb emission-line profiles
- First Results from the Lick AGN Monitoring Project: The Mass of the Black Hole in Arp 151
- VLT/ISAAC Spectra of the H-beta Region in Intermediate Redshift Quasars
- Spectral Properties From Lyman-alpha to H-alpha For An Essentially Complete Sample of Quasars I: Data
- VLT/ISAAC Spectra of the H-beta Region in Intermediate-Redshift Quasars II. Black Hole Mass and Eddington Ratio
- Observations of OI and CaII Emission Lines in Quasars: Implications for the Site of FeII Line Emission
- Low-Ionization Emission Regions in Quasars: Gas Properties Probed with Broad O I and Ca II Lines
- Close supermassive binary black holes
- The Case for Optically-Thick High Velocity Broad Line Region Gas in Active Galactic Nuclei
- HST Images and KPNO Spectroscopy of the Binary Black Hole Candidate SDSS J153636.22+044127.0
- Balmer Emission Line Profiles and the Complex Properties of Broad Line Regions in Active Galactic Nuclei
- The Redshifted Excess in Quasar C IV Broad Emission Lines
- Complex Broad Emission Line Profiles of AGN - Geometry of the Broad Line Region
- Arp 194: Evidence of Tidal Stripping of Gas and Cross-Fueling
- Accretion onto Supermassive Black Holes in Quasars: Learning from Optical/UV Observations
- Our Search for an H-R Diagram of Quasars
- The Broad Line Region of Quasars
- partly obscured accretion disk model to explain Shifted broad Balmer emission lines of Active Galactic Nuclei
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