Investigation of the angular structure of radio emission from the quasar 3C196

Details Investigation of the angular structure of radio emission from the quasar 3C196 Investigation of the angular structure of radio emission from the quasar 3C196

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990raf....33..523m&link_type=abstract

Radiofizika (ISSN 0021-3462), vol. 33, May 1990, p. 523-533. In Russian.

Physics

1

Brightness Distribution, Energy Spectra, Nebulae, Quasars, Radio Emission, Decametric Waves, Radio Interferometers, Wavelengths

Scientific paper

Angular dimensions and spectral characteristics are determined for the components of the most plausible model for brightness distribution of the quasar 3C196 at decameter and shorter wavelengths, and results are discussed. Physical processes that might be responsible for the extended region of radio emission that has been detected in 3C196 at decameter and shorter wavelengths are discussed, and it is pointed out that most previous work links such phenomena with the presence of nebulae.

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