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Crab Nebula PulsarNP 0532

Naturevolume 221, pages453–454 (1969)Cite this article

Abstract

BECAUSE of the conjecture that pulsars are neutron stars, which are possibly produced in supernova events, the possible association of pulsars with supernova remnants is of great interest. Staelin and Reifenstein recently reported1 the discovery of two pulsed radio sources near the Crab nebula, which is the remnant of the supernova observed by the Chinese in AD 1054. Pulses from both sources were described as very sporadic, and no periodic phenomena were evident.

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References

  1. IAU Circular No. 2110 (1968).

  2. Lyne, A. G., and Rickett, B. J.,Nature,218, 934 (1968).

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  3. Staelin, D. H., and Reifenstein, E. C.,Science (in the press).

  4. Large, M. I., Vaughan, A. E., and Mills, B. Y.,Nature,220, 340 (1968).

    Article ADS  Google Scholar 

  5. Gold, T.,Nature,218, 73 (1968).

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  6. Hewish, A., and Okoye, S. E.,Nature,203, 171 (1964).

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Author information

Authors and Affiliations

  1. Cornell-Sydney University Astronomy Center, Arecibo Ionospheric Observatory, Arecibo, Puerto Rico

    J. M. COMELLA, H. D. CRAFT jun., R. V. E. LOVELACE & J. M. SUTTON

  2. Center for Radar Astronomy, Stanford University, Stanford, California

    G. LEONARD TYLER

Authors
  1. J. M. COMELLA
  2. H. D. CRAFT jun.
  3. R. V. E. LOVELACE
  4. J. M. SUTTON
  5. G. LEONARD TYLER

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