Variability of the broad line spectrum of Markarian 372

Details Variability of the broad line spectrum of Markarian 372 Variability of the broad line spectrum of Markarian 372

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aj....102.1977g&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 102, Dec. 1991, p. 1977-1979.

Astronomy and Astrophysics

Astronomy

5

Active Galactic Nuclei, Galactic Radiation, Markarian Galaxies, Seyfert Galaxies, H Lines, Line Spectra

Scientific paper

Spectroscopic observations of the AGN galaxy Mrk 372 are reported. In 1986 the spectrum was that of a Seyfert type 1.5 with very broad permitted lines and modestly broadened forbidden lines. In 1990 the spectrum is that of a Seyfert type 1.9. At H-beta, the broad line component disappeared leaving only a very weak, narrow line. Observations near H-alpha, however, do reveal the presence of a broad component.

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