Considerations of the spectra of 3 CR Radio Sources

Details Considerations of the spectra of 3 CR Radio Sources Considerations of the spectra of 3 CR Radio Sources

May 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....75..240h&link_type=abstract

Astronomy and Astrophysics, vol. 75, no. 1-2, May 1979, p. 240-242.

Astronomy and Astrophysics

Astronomy

Emission Spectra, Quasars, Radio Galaxies, Radio Sources (Astronomy), Distribution Functions, Histograms, Radio Emission, Radio Spectra, Spectrum Analysis

Scientific paper

The spectra of convex unresolved 3 CR Radio Sources are considered with the aim of studying their steepenings (or breaks), perhaps the most important signature of the radiation mechanism. It is found that, although an average steepening of about 0.5 is consistent with the data, a better fit is obtained with a bimodal distribution, with the first steepening about equal to 0.35 and the second about equal to 0.70. Some implications are discussed in connection with this result, and a check made with 99 Parkes Radio Sources seems to support it.

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