Photoionized and shocked gas in active galactic nuclei

Details Photoionized and shocked gas in active galactic nuclei Photoionized and shocked gas in active galactic nuclei

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pasp...98..965v&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 98, Oct. 1986, p. 965-967.

Astronomy and Astrophysics

Astronomy

1

Active Galactic Nuclei, Emission Spectra, Interstellar Gas, Photoionization, Line Spectra, Shock Fronts

Scientific paper

The authors present an overview of the theoretical models for the narrow-emission-line region of the active galactic nuclei which take into account the coupled effect of shocks and photoionization. From the emission-line intensities previously obtained, the [O III] λ5007 line profile is calculated assuming, for a given object, that the emitting clouds have different velocities and are illuminated by the ionizing radiation with different intensities.

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