Emission line variability in NGC 4593 and NGC 5548
Abstract
Intensity and profile variations of the Balmer emission lines in the Seyfert galaxies NGC 4593 and NGC 5548 are discussed. These spectra were obtained in international monitoring campaigns. The broad line profiles consist of at least three components. These components vary independently. The FWZI of the broad line profiles remained constant during the variations.
- Publication:
-
Astrophysics and Space Science
- Pub Date:
- July 1993
- DOI:
- 10.1007/BF00657974
- Bibcode:
- 1993Ap&SS.205..179K
- Keywords:
-
- Balmer Series;
- Emission Spectra;
- Seyfert Galaxies;
- Spectral Line Width;
- Line Shape;
- Variability;
- Astrophysics