Composite models for the narrow line regions of active galactic nuclei. II - The UV lines

Details Composite models for the narrow line regions of active galactic nuclei. II - The UV lines Composite models for the narrow line regions of active galactic nuclei. II - The UV lines

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...140..368a&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 140, no. 2, Nov. 1984, p. 368-372. Research supported by the Conselho Nacional

Mathematics

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14

Active Galactic Nuclei, Astronomical Models, Line Spectra, Ultraviolet Spectra, Emissivity, Ionizing Radiation

Scientific paper

UV line calculations for the narrow line regions of active galactic nuclei are presented as part of a composite theoretical model of active galactic nuclei. Line ratios in the UV are calculated for different values of radiation flux, the spectral index, shock velocity and the cutoff energy. The results are given with the aim of explaining future observations and of supplying the narrow line core contribution to the lines which permits a more reliable fitting of the line ratios to observational results. An 'ideal' procedure is recommended for fitting the theoretical calculations to current observational data for AGN spectral emissions.

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