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The majority of the known discrete radio sources are extragalactic.
Radio sources produce either continuum radiation or line radiation.
These regularly ticking astronomical radio sources caused a sensation when they were discovered in 1967.
The purpose of the VLA is to obtain extremely high-resolution imaging of cosmic radio sources.
In the 1950s, astronomers at Cambridge University published three catalogs of astronomical radio sources.
Radio telescopes permit astronomers to study many kinds of extraterrestrial radio sources.
Within 40 years, about 100,000 such radio sources had been cataloged.
Objects like 3C 273 were called quasi-stellar radio sources, or quasars.
(For more-specific information about quasars and other extragalactic radio sources, see galaxy: Quasars).
To map such distant radio sources as quasars, Ryle developed a technique called aperture synthesis.
Differential VLBI Radio sources called VRAD experiment involves two on-board sub-satellites, Rstar and Vstar.
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