Spectrscopic monitoring of active galactic nuclei. 3: Size of the broad line region in NGC 3227

Details Spectrscopic monitoring of active galactic nuclei. 3: Size of the broad line region in NGC 3227 Spectrscopic monitoring of active galactic nuclei. 3: Size of the broad line region in NGC 3227

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26a...282..742s&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 282, no. 3, p. 742-752

Astronomy and Astrophysics

Astrophysics

37

Active Galactic Nuclei, Astronomical Spectroscopy, Balmer Series, Emission Spectra, H Alpha Line, H Beta Line, Light Curve, Visible Spectrum

Scientific paper

We present in this work the results of a five-month monitoring campaign of the active galactic nucleus in NGC 3227. Both the Balmer H-beta and H-alpha emission lines, as well as the optical continuum have been analyzed. A deblending procedure has been applied which allows for the separation of the contributions to the line emssion from the narrow line region (NLR) on one side and from the broad line region (BLR) on the other side.

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