Radio telescopes of large resolving power

Details Radio telescopes of large resolving power Radio telescopes of large resolving power

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sci...188.1071r&link_type=abstract

Science, vol. 188, June 13, 1975, p. 1071-1079.

Astronomy and Astrophysics

Astronomy

5

Antenna Arrays, Astronomical Maps, Extragalactic Radio Sources, High Resolution, Radio Galaxies, Radio Telescopes, Antenna Design, Dipole Antennas, Parabolic Antennas, Polarization Characteristics, Radio Astronomy

Scientific paper

The method of aperture synthesis is discussed, and several facilities using the method, as well as some results obtained with them, are described. A brief historical view of the development leading up to the design of aperture synthesis telescopes is given. Apparatus described includes the one-arm, one-movable-point telescope built by Blythe in 1954 and the half-mile, one-mile, and 5-km telescopes. Data are reported on the ionized hydrogen cloud NGC 7538, the powerful radio galaxy in the constellation Cygnus, polarization of the emission from the north component of the Cygnus source, and maps of six other extragalactic radio sources.

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