Spectral variations of Markarian 335

Details Spectral variations of Markarian 335 Spectral variations of Markarian 335

Nov 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86.1595s&link_type=abstract

Astronomical Journal, vol. 86, Nov. 1981, p. 1595-1599.

Astronomy and Astrophysics

Astronomy

20

Astronomical Spectroscopy, Emission Spectra, Line Spectra, Periodic Variations, Seyfert Galaxies, Balmer Series, Optical Density, Oxygen Ions, Resonance Fluorescence, Resonance Lines

Scientific paper

Mrk 335 is found to be a variable Seyfert 1 galaxy whose continuum, emission lines and 3000-A bump have varied over a two-year period (1974 to 1976). While these observations seem consistent with the existence of some optical depth in the lower-series Balmer lines, they may also indicate that the Balmer continuum is optically thin, to account for the Balmer line variations and the 3000-A bump. Additional contributions to the bump may come from the Bowen resonance-fluorescence O III lines.

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