The radio continuum emission of bright galaxies with Liner nuclei

Details The radio continuum emission of bright galaxies with Liner nuclei The radio continuum emission of bright galaxies with Liner nuclei

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...194..102g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 194, no. 1-2, April 1988, p. 102-106. Research supported by the Ministero dell

Astronomy and Astrophysics

Astrophysics

5

Brightness Distribution, Galactic Nuclei, H Ii Regions, Radio Emission, Spiral Galaxies, H Alpha Line, Seyfert Galaxies

Scientific paper

The authors have compared the radio continuum emission of about 80 bright galaxies containing LINER (low-ionization) nuclei with that of a comparable number of bright spirals having H II-region like nuclei. It is found that the former class of objects (the galaxies with LINER nuclei) tends to display, on average, weaker total radio emission (per unit light) than the latter.

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