6 CM observations of LBDS radio sources - Radio properties of blue radio galaxies

Details 6 CM observations of LBDS radio sources - Radio properties of blue radio galaxies 6 CM observations of LBDS radio sources - Radio properties of blue radio galaxies

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...192...42o&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 192, no. 1-2, March 1988, p. 42-52.

Astronomy and Astrophysics

Astrophysics

6

Astronomical Spectroscopy, Radio Galaxies, Radio Spectra, Spectrum Analysis, Galactic Structure, Radiant Flux Density, Spectral Energy Distribution

Scientific paper

The results of 6 cm observations of sources detected at 21 cm in the Leiden-Berkeley Deep Survey are used to study the radio spectra of blue radio galaxies. The mean spectral index between 6 and 21 cm of the present sources is found to be steep. The blue radio galaxies are shown to fall into two classes, those with radio morphologies similar to those of classical red radio galaxies, and those which are very compact. Both sets of characteristics can be interpreted as being typical of small optically thick nonthermal cores no more than a few parsec in size.

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