Emission line variability in NGC 4593 and NGC 5548

Details Emission line variability in NGC 4593 and NGC 5548 Emission line variability in NGC 4593 and NGC 5548

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205..179k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 1, p. 179-184.

Astronomy and Astrophysics

Astrophysics

2

Balmer Series, Emission Spectra, Seyfert Galaxies, Spectral Line Width, Line Shape, Variability

Scientific paper

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.

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