Determination of Accretion Disc Parameters in the Case of Five AGN with Double-peaked Lines

Details Determination of Accretion Disc Parameters in the Case of Five AGN with Double-peaked Lines Determination of Accretion Disc Parameters in the Case of Five AGN with Double-peaked Lines

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..938...94g&link_type=abstract

SPECTRAL LINE SHAPES IN ASTROPHYSICS: VI Serbian Conference on Spectral Line Shapes in Astrophysics (VI SCSLSA). AIP Conference

Astronomy and Astrophysics

Astrophysics

Galactic Nuclei, Circumnuclear Matter, And Bulges, Infall, Accretion, And Accretion Disks

Scientific paper

Using double-peaked lines and assuming that they are emitted from an accretion disc, it is possible to get impression about accretion disc parameters (inner and outer radius, inclination). Here we will present an analysis of accretion disc parameters obtained from five Active Galactic Nuclei (AGN) with double-peaked lines from the SDSS. The aim of this work is to connect the disc parameters with other characteristics of the host galaxy.

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