Comparing Hbeta Line Profiles in the 4D Eigenvector 1 Context
arXiv:0911.4220 · doi:10.1016/j.newar.2009.06.001
Abstract
We describe a 4D Eigenvector 1 (4DE1) space that serves as a surrogate H-R diagram for quasars. It provides a context for describing and unifying differences between all broad line AGN. Quasar spectra can be averaged in a non-random way using 4DE1 just as stellar spectra can be averaged non-randomly within the OBAFGKM classification sequence. We find that quasars with FWHM H_beta less than (Population A) and greater than (Population B) 4000 km/s show many significant differences that may point to an actual dichotomy. Broad line profile measures and fits reenforce the idea of a dichotomy because they are fundamentally different: Pop.A - Lorentzian-like and Pop.B - double Gaussian. The differences have implications both for BH mass estimation and for inferences about source structure and kinematics.
11 pages, 4 figures
References in corpus (6)
- A Comprehensive Study of 2 000 Narrow Line Seyfert 1 Galaxies from the Sloan Digital Sky Survey: I. The Sample
- CIV 1549 as an Eigenvector 1 Parameter for Active Galactic Nuclei
- A Systematic Analysis of Fe II Emission in Quasars: Evidence for Inflow to the Central Black Hole
- New Insights on the QSO Radio-Loud/Radio-Quiet Dichotomy: SDSS Spectra in the Context of the 4D Eigenvector1 Parameter Space
- VLT/ISAAC Spectra of the Hbeta Region in Intermediate-Redshift Quasars III. Hbeta Broad Line Profile Analysis and Inferences about BLR Structure
- Observational Constraints on the Dependence of Radio-Quiet Quasar X-ray Emission on Black Hole Mass and Accretion Rate
Cited by in corpus (17)
- Analysis of optical Fe II emission in a sample of AGN spectra
- Spectral Optical Monitoring of the Narrow Line Seyfert 1 galaxy Ark 564
- Modelling of the quasar main sequence in the optical plane
- The UV and optical Fe II emission lines in type 1 AGNs
- Current and future applications of Reverberation-mapped quasars in Cosmology
- A New Iron Emission Template for Active Galactic Nuclei. I. Optical Template for the H region
- The rise and fall of the iron-strong nuclear transient PS16dtm
- Spectral Evolution in High Redshift Quasars from the Final BOSS Sample
- The analysis of the hydrogen broad Balmer line ratios: possible implications to the physical properties of the BLR of AGN
- The intrinsic Baldwin effect in broad Balmer lines of six long-term monitored AGNs
- Optical emission line properties of a sample of the broad-line AGNs: the Baldwin effect and eigenvector 1
- High Metal Content of Highly Accreting Quasars: Analysis of an Extended Sample
- SALT long-slit spectroscopy of CTS C30.10: two-component Mg II line
- Line shifts and sub-pc super-massive binary black holes
- SALT long-slit spectroscopy of HE 0435-4312: fast displacement in the Mg II emission line
- A comparative study of the physical properties for a representative sample of Narrow and Broad-line Seyfert galaxies
- AGN orientation through the spectroscopic correlations and model of dusty cone shell