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Published June 1, 1974 | Published
Journal Article Open

Fine Structure in Radio Sources at 81.5 MHz-III: The Survey

Abstract

A survey of radio sources which exhibit interplanetary scintillations has been carried out with the Cambridge 18 000 m² array at 81.5 MHz. The methods of observation, and of determination of angular structure on a scale 0″.2 to 2″.0, are discussed and a catalogue lists the structure of ∼ 1500 4C sources between declinations −12° and +90°, roughly 60 per cent of which scintillate. An analysis of the results will be presented elsewhere.

Additional Information

© 1974 Royal Astronomical Society. Provided by the NASA Astrophysics Data System. (Received 1973 August 30) The full text of the above appeared in Memoirs of the Royal Astronomical Society, Volume 78, Part I.

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