Evidence for an intermediate line region in AGN's inner torus region and its evolution from narrow to broad line Seyfert I galaxies
Ling Zhu, Shuang Nan Zhang, Sumin Tang

TL;DR
This study provides evidence for an intermediate line region in AGN's inner torus, suggesting a two-component model for the broad line region that explains AGN evolution from narrow to broad line Seyfert I galaxies.
Contribution
The paper confirms the two-component BLR model using SDSS data and explores the geometry, density, and evolution of the VBLR and IMLR regions in AGNs.
Findings
Support for the two-component BLR model from SDSS data.
The IMGC affects black hole mass measurements.
Evolution from NLS1s to BLS1s explained by the model.
Abstract
A two-components model for Broad Line Region (BLR) of Active Galactic Nuclei (AGN) has been suggested for many years but not widely accepted (e.g., Hu et al. 2008; Sulentic et al. 2000; Brotherton et al. 1996; Mason et al. 1996). This model indicates that the broad line can be described with superposition of two Gaussian components (Very Broad Gaussian Component (VBGC) and InterMediate Gaussian Component (IMGC)) which are from two physically distinct regions; i.e., Very Broad Line Region (VBLR) and InterMediate Line Region (IMLR). We select a SDSS sample to further confirm this model and give detailed analysis to the geometry, density and evolution of these two regions. Micro-lensing result of BLR in J1131-1231 and some unexplained phenomena in Reverberation Mapping (RM) experiment provide supportive evidence for this model. Our results indicate that the radius obtained from the…
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