A plasmon driven bowshock model for the narrow line region of NGC 5929

Details A plasmon driven bowshock model for the narrow line region of NGC 5929 A plasmon driven bowshock model for the narrow line region of NGC 5929

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.240..487t&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 240, Sept. 15, 1989, p. 487-499.

Astronomy and Astrophysics

Astronomy

41

Bow Waves, Galactic Nuclei, Line Spectra, Plasmons, Seyfert Galaxies, Shock Waves, Astronomical Models, Extragalactic Radio Sources, Line Shape, Photoionization

Scientific paper

A model for the narrow line region (NLR) of Seyfert nuclei, in which the linear motion of radio-emitting bubbles of plasma ejected from the nucleus drives bowshocks into the ambient nuclear medium is described. The cooled shocked gas, photoionized by the UV nuclear continuum, produces the optical NLR emission. This provides a natural explanation for the relationship between the radio continuum emission and the NLR. This is then applied to the NLR of the Seyfert 2 galaxy NGC 5929.

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