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.
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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).
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BAILEY, J., MACKAY, C. Accurate Position of a Second Pulsed Radio Source. Nature 218, 129–130 (1968). https://doi.org/10.1038/218129a0
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DOI: https://doi.org/10.1038/218129a0
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