Shock and photoionization models for infrared lines from active galactic nuclei

Details Shock and photoionization models for infrared lines from active galactic nuclei Shock and photoionization models for infrared lines from active galactic nuclei

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205..149c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 1, p. 149-154.

Astronomy and Astrophysics

Astrophysics

Active Galactic Nuclei, Astronomical Models, Emission Spectra, Infrared Spectra, Photoionization, Shock Wave Propagation, Line Spectra, Power Series, Supernova Remnants

Scientific paper

IR lines are calculated for AGN by SVMA code. IR line ratios, as
temperature and density diagnostic of the emitting gas, show that the
forbidden S III line ratio increases with shock velocity, following
compression and cooling of the gas downstream. The results are compared
with observations and briefly discussed.

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