The structure of radio sources 3C 273B and 3C 84 deduced from the 'closure' phases and visibility amplitudes observed with three-element interferometers

Astronomy and Astrophysics – Astronomy

Scientific paper

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87

Brightness, Extragalactic Radio Sources, Interferometry, Microwave Interferometers, Quasars, Radio Astronomy, Data Reduction, Fourier Series, Phase Shift, Radiant Flux Density, Seyfert Galaxies, Spatial Distribution, Visibility

Scientific paper

The derived 'closure' phase relation for a three-element interferometer is used in a presented analysis of data obtained from observations at 7.8 GHz of the radio sources 3C 273B and 3C 84 by antennas in Massachusetts, California, Alaska, and Sweden (the first two antennas were used in combination with each of the last two separately to form two three-element interferometers). The brightness distribution is found for each source by expansion of both the fringe amplitude and the fringe phase in separate Fourier series.

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