The radio emission of galaxies with low-luminosity active nuclei

Details The radio emission of galaxies with low-luminosity active nuclei The radio emission of galaxies with low-luminosity active nuclei

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.157..255g&link_type=abstract

(Instituto de Astrofisica de Canarias and Comision Interministerial de Ciencia y Tecnologia, Summer School on Evolutionary Pheno

Astronomy and Astrophysics

Astrophysics

Active Galactic Nuclei, Galactic Radio Waves, Seyfert Galaxies, Continuous Spectra, H Ii Regions, Luminosity

Scientific paper

The radio continuum emission of three samples of bright galaxies are compared with LINER, H II region-like, and Seyfert nuclei. Basically, it is found that the objects of the first class are the weakest total and central radio emitters (for total and central unit light, respectively), whereas the Seyfert galaxies contain the most powerful central radio sources.

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