The radio structure of radio loud and radio quiet quasars in the Palomar Bright Quasar Survey

Details The radio structure of radio loud and radio quiet quasars in the Palomar Bright Quasar Survey The radio structure of radio loud and radio quiet quasars in the Palomar Bright Quasar Survey

Oct 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994aj....108.1163k&link_type=abstract

The Astronomical Journal, vol. 108, no. 4, p. 1163-1177

Astronomy and Astrophysics

Astronomy

130

Active Galactic Nuclei, Galactic Structure, Quasars, Radio Astronomy, Radio Galaxies, Radio Spectra, Radio Stars, Sky Surveys (Astronomy), Stellar Luminosity, Stellar Spectra, Astronomical Spectroscopy, Emission Spectra, Radio Spectroscopy, Radio Telescopes

Scientific paper

Images of resolved radio sources in the Palomar Bright Quasar Survey (BQS) are presented with an angular resolution of 0.5 and 18 arcsec. The observed structure of some well resolved radio quiet quasars and active galactic nuclei (AGN) show large scale linear structures or unresolved central cores similar to radio loud objects in the BQS sample as well as the more luminous radio selected quasars. We suggest that at least some of these less luminous radio quiet objects may contain compact central engines characteristic of radio loud quasars and radio galaxies.

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