The Origin of Fe II Emission in AGN

Details The Origin of Fe II Emission in AGN The Origin of Fe II Emission in AGN

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..311..419b&link_type=abstract

AGN Physics with the Sloan Digital Sky Survey, Proceedings of a conference held in Princeton, NJ, USA, 27-31 July 2003, Edited b

Physics

Scientific paper

We use Cloudy models to investigate the physical process by which the Fe
II emission lines in AGN are formed. If Fe II comes from photoionized
gas, significant microturbulence is required. Alternatively, the lines
may come from a fairly hot collisionally excited gas.

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