Double- (and Single-) Peaked Emission Lines as Probes of the Structure of the Outer Accretion Disks in AGN

Details Double- (and Single-) Peaked Emission Lines as Probes of the Structure of the Outer Accretion Disks in AGN Double- (and Single-) Peaked Emission Lines as Probes of the Structure of the Outer Accretion Disks in AGN

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008rmxac..32...50f&link_type=abstract

The Nuclear Region, Host Galaxy and Environment of Active Galaxies (Eds. Erika Benítez, Irene Cruz-González, & Yair Krongold) Re

Physics

Galaxies: Active, Black Hole Physics

Scientific paper

Broad, double-peaked Balmer emission lines provide dynamical evidence
for the presence of an accretion disk feeding a supermassive black hole
in the central engines of AGN.

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