8.4 GHz VLA observations of the CfA Seyfert sample

Details 8.4 GHz VLA observations of the CfA Seyfert sample 8.4 GHz VLA observations of the CfA Seyfert sample

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.216..371k&link_type=abstract

Astrophysics and Space Science, vol. 216, no. 1-2, p. 371-372

Astronomy and Astrophysics

Astronomy

Astronomical Models, Galactic Structure, Radio Astronomy, Radio Jets (Astronomy), Seyfert Galaxies, Sky Surveys (Astronomy), Active Galactic Nuclei, Emission Spectra, Line Spectra, Stellar Luminosity, Very Large Array (Vla)

Scientific paper

We present the results of an 8.4 GHz very large array (VLA) survey of the CfA Seyferts. We find that the luminosity functions for Seyfert 1s and 2s are essentially identical, but that the type 2 objects are more likely to contain extended radio structures. This seems to be consistent with unified models for Seyferts, in which the differences between the two classes are largely due to orientation effects.

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