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Fluorescence in the Active Galactic Nuclei NGC 4151
Published online by Cambridge University Press: 17 July 2013
Abstract
The possibility of UV lines from Fe II formed in the BLR of NGC 4151 has been examined. As a result Fe II emission has been shown to play an important role for the topology of the 2000 to 3000 Å wavelength region of the NGC 4151 spectra. The Fe II UV emission originates from two processes, collisional excitation and PAR (photoexcitation by accidental resonance).
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- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 8 , Symposium S295: The intriguing life of massive galaxies , August 2012 , pp. 266
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- Copyright © International Astronomical Union 2013