Radio Seyferts and the forbidden line region

Details Radio Seyferts and the forbidden line region Radio Seyferts and the forbidden line region

Oct 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984xue..conf...14p&link_type=abstract

In Max-Planck Inst. für Physik und Astrophysik X-Ray and UV Emission from Active Galactic Nuclei p 14-17 (SEE N85-17790 08-88)

Astronomy and Astrophysics

Astrophysics

1

Galactic Nuclei, Galactic Radio Waves, Interstellar Gas, Line Spectra, Radio Spectra, Seyfert Galaxies, Astronomical Models, Interstellar Radiation, Interstellar Space, Radio Galaxies, Shock Waves

Scientific paper

A model in which the expansion of the radio emitting components in Seyfert 2 nuclei compress and accelerate the ambient medium by means of shock waves is described. When the expansion velocity of the component decreases to 400 km/sec, the compressed gas cools and radiates producing the forbidden line region. This readily accounts for the intimate relationship between the radio continuum emission and the properties of the forbidden line region.

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