Abstract
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.
Original language | English |
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Pages (from-to) | 742-752 |
Journal | Astronomy and Astrophysics |
Volume | 282 |
Publication status | Published - 1 Feb 1994 |
Keywords / Materials (for Non-textual outputs)
- Active Galactic Nuclei
- Astronomical Spectroscopy
- Balmer Series
- Emission Spectra
- H Alpha Line
- H Beta Line
- Light Curve
- Visible Spectrum