The behavior of hot spots in classical double radio sources

Details The behavior of hot spots in classical double radio sources The behavior of hot spots in classical double radio sources

Aug 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..531n&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Aug. 1980, p. 531-544.

Astronomy and Astrophysics

Astronomy

14

Binary Stars, Extragalactic Radio Sources, Stellar Luminosity, Stellar Structure, Brightness Temperature, Correlation Coefficients, Data Processing, Red Shift, Stochastic Processes, Surface Properties, Void Ratio

Scientific paper

The relationship between the structure and luminosity of strong extragalactic radio sources (reported by Jenkins & McEllin) and between the source structure and redshift is shown to be largely an effect of observing the sources with unequal linear resolutions. Weak trends still exist after statistical correction for resolution effects, but they are dominated by inter- and intra-source scatter. At 5-km resolution, the fraction of total flux which comes from 'hot spots' of high surface brightness could be dependent on some as-yet-undetermined source characteristics, or it could be caused by some short-lived stochastic process that is unrelated in detail to general source properties.

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