Radio structure of the M87 jet

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Astronomical Models, Extragalactic Radio Sources, Galactic Radio Waves, Galactic Structure, Microwave Interferometers, Galactic Nuclei, Radio Emission, Radio Relay Systems, Spatial Distribution, Synchrotron Radiation

Scientific paper

Interferometer observations at 408 and 1666 MHz with resolving powers of approximately 0.5 sec along the jet are reported. To compensate for changes in link path delay due to atmospheric changes the 1666 MHz interferometer uses an improved radio link system. Direct Fourier inversion of the 1666 MHz amplitude and phase data is used to obtain strip distributions in right ascension to show other compact components in the sources. A model-fitting technique which assumes that the components have Gaussian symmetry is used to analyze fringe amplitude data. Results show that the electrons involved in radio and optical synchrotron emission have similar spatial distributions.

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