Astronomy and Astrophysics – Astrophysics
Scientific paper
Nov 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...168...41c&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 168, no. 1-2, Nov. 1986, p. 41-48.
Astronomy and Astrophysics
Astrophysics
20
Astronomical Models, Galactic Nuclei, Seyfert Galaxies, Spectral Line Width, Spectrum Analysis, Active Galactic Nuclei, Astronomical Spectroscopy, Emission Spectra, Photoionization, Shock Waves
Scientific paper
In this paper the analysis of the emission line spectra of Seyfert galaxies is continued in the light of the composite models for the narrow line region of active galactic nuclei. The model accounts for the coupled effect of photoionization and shock waves in determining the physical conditions in the emitting clouds. Therefore, some calculations about densities and temperatures in the postshock region are presented in the range of the observed values, and correlations with shock velocities are discussed. The observed data of a particular group of galaxies, called intermediate Seyfert galaxies (Cohen, 1983) are compared to model calculations. From the point of view of narrow lines, the results show that Seyfert type 2, intermediate Seyfert galaxies, and Liners may be interpreted as different aspects of the same phenomenon, depending only on the relative importance of photoionization and shock effects in determining the physical conditions of the emitting region.
Aldrovandi M. V. S.
Contini Marcella
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