BLR: Non-radiative Heating in Strong Fe II Emitters

Details BLR: Non-radiative Heating in Strong Fe II Emitters BLR: Non-radiative Heating in Strong Fe II Emitters

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..373..376j&link_type=abstract

The Central Engine of Active Galactic Nuclei, ASP Conference Series, Vol. 373, proceedings of the conference held 16-21 October,

Physics

Scientific paper

The optical spectrum of Seyfert 1s reveals a great variety in the Fe II
emission. We investigate the formation of these lines in some strong Fe
II emitters and determine the physical conditions of the emission
region. We show the need of a non-radiative heating to account for the
observations.

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