Resolution of celestial radio sources with super-synthesis VLBI

Details Resolution of celestial radio sources with super-synthesis VLBI Resolution of celestial radio sources with super-synthesis VLBI

Sep 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978rarlr..24..577t&link_type=abstract

Radio Research Laboratories, Review, vol. 24, Sept. 1978, p. 577-590. In Japanese.

Astronomy and Astrophysics

Astronomy

Antenna Radiation Patterns, High Resolution, Radio Sources (Astronomy), Spaceborne Astronomy, Synthetic Arrays, Very Long Base Interferometry, Computerized Simulation, Radio Astronomy, Radio Stars, Satellite Antennas, Spectral Resolution, Synchronous Satellites

Scientific paper

Some examples of celestial radio sources recently resolved by VLBI observations (especially by the use of the phase closure method) are given, including 3C273B, 3C84, and 3C147. Computer simulations of beam patterns formed by two or three antennas are discussed along with some theoretical formulas. It is concluded that VLBI with antennas mounted on synchronous satellites will make it possible to observe radio stars with high resolution in the hectometric region.

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