Far infrared fine structure lines in active galaxies

Details Far infrared fine structure lines in active galaxies Far infrared fine structure lines in active galaxies

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.290..525s&link_type=abstract

In ESA, Infrared Spectroscopy in Astronomy p 525-529 (SEE N90-19084 11-89)

Astronomy and Astrophysics

Astronomy

1

Active Galaxies, Far Infrared Radiation, Fine Structure, Infrared Spectra, Astronomical Models, European Space Programs, Infrared Space Observatory (Iso), Line Spectra, Photoionization

Scientific paper

The line fluxes of the far infrared fine structure ionic and atomic transitions in the narrow line regions of active galaxies are predicted. A standard photoionization model is used. Data from the observed flux of the Seyfert 2 galaxy NGC 1068 is analyzed. The standard conditions in active galaxies narrow line regions are assumed. The (C II) 158 microns, (O I) 63 microns, (N III) 57 microns, (N II) 122 microns and (O III) 88 microns and 52 microns are detectable at high resolution (R=10,000) with the long wavelength spectrometer, on board the ESA satellite Infrared Space Observatory.

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