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

Readhead, A. C. S. and Hewish, A. (1974) Fine Structure in Radio Sources at 81.5 MHz-III: The Survey. Monthly Notices of the Royal Astronomical Society, 167 (3). p. 663. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200601-143024614

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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.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/167.3.663DOIArticle
https://ui.adsabs.harvard.edu/abs/1974MNRAS.167..663R/abstractADSArticle
ORCID:
AuthorORCID
Readhead, A. C. S.0000-0001-9152-961X
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.
Issue or Number:3
Record Number:CaltechAUTHORS:20200601-143024614
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200601-143024614
Official Citation:A. C. S. Readhead, A. Hewish, Fine Structure in Radio Sources at 81.5 MHz–III: T HE S URVEY, Monthly Notices of the Royal Astronomical Society, Volume 167, Issue 3, June 1974, Page 663, https://doi.org/10.1093/mnras/167.3.663
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103613
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:01 Jun 2020 22:31
Last Modified:01 Jun 2020 22:31

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