Abstract
The Cambridge one-mile telescope has been used to fix the position of a second pulsed radio source. There is no obvious identification with an optical source.
Similar content being viewed by others
References
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature, 217, 709 (1968).
Ryle, M., and Bailey, J. A., Nature, 217, 907 (1968).
Longair, M. S., Mon. Not. Roy. Astro. Soc., 129, 419 (1965).
Allen, C. W., Astrophysical Quantities (Athlone Press, 1963).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
BAILEY, J., MACKAY, C. Accurate Position of a Second Pulsed Radio Source. Nature 218, 129–130 (1968). https://doi.org/10.1038/218129a0
Received:
Issue Date:
DOI: https://doi.org/10.1038/218129a0
- Springer Nature Limited
This article is cited by
-
Preliminary Results on Pulsating Radio Sources
Nature (1968)
-
Proper Motion Search for Pulsars
Nature (1968)
-
Accurate Positions of CP0950 and CP1133
Nature (1968)
-
Nature of the Pulsating Radio Sources
Nature (1968)
-
A Pulsar Supernova Association?
Nature (1968)