The influence of relativistic electrons on a photoionized gaseous cloud

Details The influence of relativistic electrons on a photoionized gaseous cloud The influence of relativistic electrons on a photoionized gaseous cloud

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...70..143g&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 70, no. 2, Aug. 1987, p. 143-156.

Astronomy and Astrophysics

Astronomy

13

Galactic Nuclei, Interstellar Gas, Photoionization, Radio Sources (Astronomy), Relativistic Electron Beams, Active Galactic Nuclei, Emission Spectra, Line Spectra

Scientific paper

A grid of models for a dilute photoionized gas cloud reached by a flux of relativistic electrons is presented. Their influence on the physical conditions of the emitting gas and on the emission line intensities is analysed. The input parameters are the elemental abundances, the hydrogen density, the ionization parameter and the flux of the relativistic electrons. These models can describe the narrow emission line region of the active galactic nuclei showing radio emission.

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