Evolution of broad-line emission from active galactic nuclei
@article{Elitzur2014EvolutionOB, title={Evolution of broad-line emission from active galactic nuclei}, author={M. Elitzur and L. Ho and J. Trump}, journal={Monthly Notices of the Royal Astronomical Society}, year={2014}, volume={438}, pages={3340-3351} }
Apart from viewing-dependent obscuration, intrinsic broad-line emission from active galactic nuclei (AGN) follows an evolutionary sequence: type 1 → 1.2/1.5 → 1.8/1.9 → 2a s the accretion rate on to the central black hole is decreasing. This spectral evolution is controlled, at least in part, by the parameter Lbol/M 2/3 , where Lbol is the AGN bolometric luminosity and M is the black hole mass. Both this dependence and the double-peaked profiles that emerge along the sequence arise naturally in… Expand
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- 36
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References
SHOWING 1-10 OF 75 REFERENCES
ON THE DISAPPEARANCE OF THE BROAD-LINE REGION IN LOW-LUMINOSITY ACTIVE GALACTIC NUCLEI
- Physics
- 2009
- 123
- PDF
Double-peaked emission lines as a probe of the broad-line regions of active galactic nuclei
- Physics
- 2009
- 39
Magnetic acceleration of broad emission-line clouds in active galactic nuclei
- Physics
- 1992
- 207
- Highly Influential