Scintillation of 3C 48, 3C 273, and 3C 295 at 25 MHz

Details Scintillation of 3C 48, 3C 273, and 3C 295 at 25 MHz Scintillation of 3C 48, 3C 273, and 3C 295 at 25 MHz

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977sva....21..540a&link_type=abstract

(Astronomicheskii Zhurnal, vol. 54, Sept.-Oct. 1977, p. 953-956.) Soviet Astronomy, vol. 21, Sept.-Oct. 1977, p. 540-542. Trans

Astronomy and Astrophysics

Astronomy

Decametric Waves, Extragalactic Radio Sources, Interplanetary Medium, Scintillation, Astronomical Models, Atmospheric Attenuation, Brightness, Halos, Oscillographs, Radio Astronomy

Scientific paper

Interplanetary scintillations of the extragalactic radio sources 3C 48, 3C 273, and 3C 295 have been observed at 25 MHz. Models of the angular structure of these sources are proposed which are in accord with the observational data. It is found that 3C 48 possesses a halo, that 3C 295 becomes a single-component source at decameter wavelengths, and that 3C 273 has the same structure at 25 MHz as at meter wavelengths.

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