Spectroscopy of the Seyfert galaxies Arakelyan 564, III Zwicky 77, and I Zwicky 92

Astronomy and Astrophysics – Astronomy

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Astronomical Spectroscopy, Emission Spectra, Line Spectra, Seyfert Galaxies, Electron Density (Concentration), Interstellar Gas, Oxygen Spectra, Red Shift, Spectral Line Width

Scientific paper

A spectroscopic analysis of the Seyfert I galaxies Ark 564 and III Zw 77 and the Seyfert 2 object I Zw 92 is described. Redshifts, equivalent widths, flux densities, and luminosities are determined for emission lines on spectrograms taken with the 2.6-m Crimean reflector. The electron density and temperature of the gas are estimated from the relative forbidden O III line intensities. Some physical parameters (volume, mass, characteristic size, kinetic energy) are evaluated for the gas responsible for the permitted and forbidden emission lines. The mass of the central body in each nucleus and the luminosity in the 3600-7000 A interval are estimated.

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