High-resolution observations of Centaurus-A and Pictor-A at 160 MHz

Details High-resolution observations of Centaurus-A and Pictor-A at 160 MHz High-resolution observations of Centaurus-A and Pictor-A at 160 MHz

Oct 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975pasau...2..336s&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 9th, Parkes, New South Wales, Australia, May 14-16, 1975.) Astronomi

Astronomy and Astrophysics

Astronomy

5

Galactic Structure, Radiant Flux Density, Radio Galaxies, Astronomical Maps, Galactic Radiation, High Resolution, Microwave Emission, Radio Astronomy

Scientific paper

The radioheliograph at Culgoora, N.S.W. was used in a study of Centaurus-A and Pictor-A. Recordings of each object were obtained on three separate nights in order to avoid distortions of the brightness contours due to ionospheric disturbances or equipment malfunction. The brightness distribution of the central components of Centaurus-A at 160 MHz is shown. The measurements confirm the conclusions of Lockhart and Sheridan (1970) that the major axis of the central components lie in position angles significantly different from the line joining their peaks. A brightness distribution of Pictor-A at 160 MHz is also presented.

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