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High-Resolution Observations of Radio Sources

Cohen, Marshall H. (1969) High-Resolution Observations of Radio Sources. Annual Review of Astronomy and Astrophysics, 7 . pp. 619-664. ISSN 0066-4146. https://resolver.caltech.edu/CaltechAUTHORS:20161019-082031869

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Abstract

Recent developments have greatly increased the angular resolution attainable in radio astronomy. The largest reflectors give a resolution of 2 to 3 min of are, close to that of the unaided human eye. Interplanetary scintillations and interferometry give 10^(-3) sec of arc and higher; this exceeds the resolution of Michelson's stellar interferometer by more than an order of magnitude, and is comparable to the highest resolution attained by the optical intensity interferometer (1).


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1146/annurev.aa.07.090169.003155DOIArticle
http://www.annualreviews.org/doi/10.1146/annurev.aa.07.090169.003155PublisherArticle
Additional Information:© 1969 Annual Reviews. I am grateful to many colleagues for supplying results in advance of their publication, and for their helpful comments. This research was sponsored by the Air Force Office of Scientific Research, Office of Aerospace Research, grant AFOSR-69-1648.
Funders:
Funding AgencyGrant Number
Air Force Office of Scientific Research (AFOSR)AFOSR-69-1648
Record Number:CaltechAUTHORS:20161019-082031869
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20161019-082031869
Official Citation:High-Resolution Observations of Radio Sources Marshall H. Cohen Annual Review of Astronomy and Astrophysics, Vol. 7: 619 -664 (Volume publication date September 1969)
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:71255
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Oct 2016 15:53
Last Modified:03 Oct 2019 16:05

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