Optical spectra of the nuclei of radio galaxies with radio jets

Details Optical spectra of the nuclei of radio galaxies with radio jets Optical spectra of the nuclei of radio galaxies with radio jets

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91..257m&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, June-July 1979, p. 257-259. Research supported by the Martin Kellog

Astronomy and Astrophysics

Astronomy

21

Astronomical Spectroscopy, Galactic Nuclei, Galactic Radiation, Radio Galaxies, Radio Jets (Astronomy), Emission Spectra, Ionization, Light (Visible Radiation), Line Spectra

Scientific paper

Emission-line optical spectra have been measured for several radio
galaxies with radio jets, including the giant radio galaxies 3C 236 and
NGC 6251. The emission lines in all these objects are relatively weak
and correspond to a lower average degree of ionization than in typical
narrow-line radio galaxies.

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