Observations with a VLB array. 2: The sources 4C39.25, NRAO150, VRO42.11.01, 3C345, and 3C454.3,342

Details Observations with a VLB array. 2: The sources 4C39.25, NRAO150, VRO42.11.01, 3C345, and 3C454.3,342 Observations with a VLB array. 2: The sources 4C39.25, NRAO150, VRO42.11.01, 3C345, and 3C454.3,342

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975stin...7523433s&link_type=abstract

Unknown

Astronomy and Astrophysics

Astronomy

Extraterrestrial Radio Waves, Radio Interferometers, Radio Sources (Astronomy), Brightness, Flux Density, Mathematical Models, Radio Emission, Radio Telescopes

Scientific paper

Three-antenna long baseline interferometry at 10.7 GHz is reported for NRAO150, 4C39.25, 3C345, VRO42.22.01, and 3C454.3 for several epochs between April, 1972 and February, 1974. Simple models for the source brightness distributions fit the observations and indicate that most of the radio emission comes from one or two components. Component separations range up to approximately 50 light years, and component sizes are on the order of 10 light years. Small variations in source structure have been observed.

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