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The accurate positions of 17 intense radio sources

Published online by Cambridge University Press:  14 August 2015

B. Elsmore
B. Elsmore*
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory Cambridge, England

Extract

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Observations of 17 intense sources were made at a 1.9-meter wavelength with the Cambridge four-aerial interferometer [1] to provide information that may assist in their identification with optical objects, and as a check on the positions of a few of the sources of the recently completed third Cambridge survey [2].

Type
Part III: Galactic and Extragalactic Radio Sources
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 337 - 338
Copyright
Copyright © Stanford University Press 1959 

References

1. Ryle, M. and Hewish, A. Mem. R.A.S. 67, 97, 1955.Google Scholar
2. Edge, D. O., Shakeshaft, J. R., Archer, S., and Baldwin, J. E. (In preparation.) Google Scholar
3. Elsmore, B. M.N.R.A.S. (In press.) Google Scholar
4. Ryle, M. Proc. Roy. Soc. Lond. A 211, 351, 1952.Google Scholar
5. Mills, B. Y., Slee, O.B., and Hill, E.R. Aust. J. Phys. 11, 360, 1958.CrossRefGoogle Scholar