A model for the complex extragalactic radio source 3C 288

Details A model for the complex extragalactic radio source 3C 288 A model for the complex extragalactic radio source 3C 288

Jun 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pasp...92..262b&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 92, June 1980, p. 262-265. Research supported by the University of Alaba

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4

Astronomical Models, Extragalactic Radio Sources, Galactic Structure, Mathematical Models, Radio Galaxies, Brightness, Intergalactic Media, Plasma Clouds, Plasma Frequencies, Spatial Distribution

Scientific paper

A method of modeling complex double radio sources and head-tail radio sources is described. The method is most easily applied to the slingshot theory of radio sources but may be used also in other theories. As an example, a model of 3C 288 based on the slingshot theory is presented and the brightness distribution at two different observing frequencies and spatial resolutions is calculated.

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