Lunar Occultation of Radio Sources
Open Access
- 1 February 1965
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 129 (2) , 199-204
- https://doi.org/10.1093/mnras/129.2.199
Abstract
A method for deriving profiles of the brightness distribution of radio sources from observations of lunar occultations has been described in an earlier paper. The method has now been applied to observations of 3C273 by Hazard, Mackey and Shimmins. The results, and some technical details concerning the method, are presented in this paper.Keywords
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