Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aj....104.2072t&link_type=abstract
Astronomical Journal (ISSN 0004-6256), vol. 104, no. 6, p. 2072-2077.
Astronomy and Astrophysics
Astronomy
30
Galactic Nuclei, Markarian Galaxies, Seyfert Galaxies, Balmer Series, Charge Coupled Devices, Emission Spectra, H Lines
Scientific paper
The nuclear spectrum of the broad-line Seyfert galaxy Mrk 993 was observed to display strong variations in the strengths of the broad H-alpha and H-beta emission lines, changing its classification from a Seyfert 1 to a Seyfert 1.9. Moderate to high resolution spectra were obtained with the IDS and CCD spectrograph on the 3 m Shane telescope at Lick Observatory in four different epochs spanning a period of approximately eight years. Using a spectral decomposition method which isolates the pure emission component of the active nucleus from the contaminating underlying host galaxy, our analysis indicates that the broad-line fluxes varied such that the Balmer decrement steepens whenever broad H-alpha and H-beta decrease in strength, and that the ionizing continuum correspondingly reddens in slope. These direct observational evidences suggest that variation in extinction along the line of sight to the broad-line region of Mrk 993 provides a simple explanation to the behavior of its spectrum, although a combination of possibilities may also be possible.
Martel Andre
Osterbrock Donald E.
Tran Hien D.
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