Experimental investigation of the angular structure of the quasar 3C196 at decameter wavelengths

Details Experimental investigation of the angular structure of the quasar 3C196 at decameter wavelengths Experimental investigation of the angular structure of the quasar 3C196 at decameter wavelengths

May 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990raf....33..534m&link_type=abstract

Radiofizika (ISSN 0021-3462), vol. 33, May 1990, p. 534-545. In Russian.

Computer Science

2

Brightness Distribution, Decametric Waves, Quasars, Radio Emission, Radio Interferometers, Energy Spectra, Radio Frequencies

Scientific paper

Angular structure of the radio emission from the quasar 3C196 was measured at 25.20 and 16.7 MHz by the URAN-1 and URAN-4 radio interferometers. The most probable model for the radio-brightness distribution consists of a single compact component and an extended component determining a significant increase in the angular size of the object.

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