MBG 02223-1922 - A newly identified luminous Seyfert galaxy

Astronomy and Astrophysics – Astronomy

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Astronomical Photometry, Forbidden Transitions, Galactic Nuclei, Seyfert Galaxies, Spectrophotometry, Visual Photometry, Cosmic Dust, Emission Spectra, Infrared Spectra, Interstellar Extinction, Luminosity, Spiral Galaxies, Star Formation

Scientific paper

Spectrophotomety in the 4300-5300 A range and direct imaging in B, V, and I of the Montreal Blue Galaxy (MBG) 02223-1922, a new, bright (V=13.5), Seyfert 1 galaxy are presented. Data obtained reveal unusually broad and composite forbidden lines, which suggests a more complex dynamical structure of the narrow-line region than is usually proposed for Seyfert galaxies. The galaxy is characterized by the moderately large infrared luminosity, L(IR)=6.6 x 10 exp 10 L solar masses, relatively flat FIR spectrum (indices alpha(12,25)=-0.98 and alpha(12, 60)=-1.33), the average value of the flux ratio, and internal reddening, E(B-V)=0.38. These parameters suggest that only a small quantity of dust is present in the nucleus. It is concluded that MBG 02223-1922 is probably a so-called Seyfert galaxy 1.8.

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