Observations with a VLB array. II - The sources 4C 39.25, NRAO 150, VRO 42.22.01, 3C 345, and 3C 454.3

Astronomy and Astrophysics – Astronomy

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Microwave Interferometers, Radiant Flux Density, Radio Sources (Astronomy), Radio Telescopes, Red Shift, Antenna Arrays, Astronomical Models, High Resolution, Microwave Antennas, Quasars, Radio Astronomy

Scientific paper

Results are reported for three-antenna long-baseline interferometric observations at 10 GHz of the cited sources. The optical identifications and redshifts of the sources are given along with their total flux densities at the epochs of the observing sessions. Small variations in source structure are noted, and simple models for the source brightness distributions are fitted to the data. The results indicate that most of all of the total 10.7-GHz flux density is supplied by two compact components with separations ranging up to approximately 50 light years and sizes of the order of 10 light years.

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