The Disk Emission in Single Peaked Lines for 12 AGNs

Details The Disk Emission in Single Peaked Lines for 12 AGNs The Disk Emission in Single Peaked Lines for 12 AGNs

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008seraj.177....9b&link_type=abstract

Serbian Astronomical Journal, vol. 177, pp. 9-13

Astronomy and Astrophysics

Astronomy

5

Galaxies: Active, Line: Formation, Plasmas

Scientific paper

The disk emission in the single peaked Broad Emission Lines (BELs) of Active Galactic Nuclei (AGNs) is difficult to detect. In order to find the disk traces in BELs the line profiles were simulated by the simplified model consisting of two components: accretion disk and surrounding spherical region with isotropic velocities of clouds. The measurements of simulated profiles were compared with the measurements of observed single-peaked Hα and Hβ profiles of 12 AGNs, that had been previously confirmed to show the accretion disk presence in the X domain. The results are in agreement with previous investigations.

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