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Pulsating Radio Source at α = 19h19m, δ = +22°

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Abstract

Signals from one of the rapidly pulsating radio sources have been recorded on three frequencies using the mark I radio telescope at the Nuffield Radio Astronomy Laboratories. The size of the source, deduced from the form of the signals, again seems consistent with an origin in a white dwarf or neutron star.

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References

  1. Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature, 217, 709 (1968).

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Authors and Affiliations

  1. University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank,

    J. G. DAVIES, P. W. HORTON, A. G. LYNE, B. J. RICKETT & F. G. SMITH

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  1. J. G. DAVIES
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  2. P. W. HORTON
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  3. A. G. LYNE
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  4. B. J. RICKETT
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  5. F. G. SMITH
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DAVIES, J., HORTON, P., LYNE, A. et al. Pulsating Radio Source at α = 19h19m, δ = +22°. Nature 217, 910–912 (1968). https://doi.org/10.1038/217910a0

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  • DOI: https://doi.org/10.1038/217910a0

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