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Pulsar Associated with the Supernova Remnant IC 443

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Abstract

DURING the period July 26 to September 21, 1972, the Jodrell Bank Mark IA radio telescope has been engaged in a systematic search for pulsars at a frequency of 408 MHz. The technique is that used by Davies, Large and Pickwick1 in 1970, but adapted in a way that allows the analysis to be carried out in real time on the Argus data processing computer.

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References

  1. Davies, J. G., Large, M. I., and Pickwick, A. C., Nature, 227, 1123 (1970).

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  2. Minkowski, R., IAU Symposium No. 46, 241 (1971).

  3. Milne, D. K., IAU Symposium No. 46, 248 (1971).

  4. Taylor, J. H., Huguenin, G. R., and Manchester, R. N., IAU Circ., 2435 (1972).

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Authors and Affiliations

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

    J. G. DAVIES, A. G. LYNE & J. H. SEIRADAKIS

Authors
  1. J. G. DAVIES
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  2. A. G. LYNE
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  3. J. H. SEIRADAKIS
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DAVIES, J., LYNE, A. & SEIRADAKIS, J. Pulsar Associated with the Supernova Remnant IC 443. Nature 240, 229–230 (1972). https://doi.org/10.1038/240229a0

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