Asymmetry of the C IV λ 1549 Å and [O III] λλ 4959, 5007 Å Lines in a Sample of RQ and RL AGN

Details Asymmetry of the C IV λ 1549 Å and [O III] λλ 4959, 5007 Å Lines in a Sample of RQ and RL AGN Asymmetry of the C IV λ 1549 Å and [O III] λλ 4959, 5007 Å Lines in a Sample of RQ and RL AGN

Sep 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..938..104k&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

Active And Peculiar Galaxies And Related Systems, Quasars

Scientific paper

Here we investigate the asymmetry of the C IV λ 1549 Å line in a sample of Radio Quiet (RQ) and Radio Loud (RL) Active Galactic Nuclei (AGN), in order to find signature of an outflow in C IV λ 1549 Å emission region. We apply two-component Gaussian analysis to fit the lines. We consider the parameters of the components (emission and absorption), separately in Radio Loud and Radio Quiet AGN, and we compared those parameters with parameters of the fits of [O III] λλ 4959, 5007 Å lines, trying to see if there is any kinematical correlation between the emission regions (HIL BLR and NLR) where C IV λ 1549 Å and [O III] λλ 4959, 5007 Å lines are formed.

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