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Abstract

PULSED optical emission has been detected from the Vela pulsar, PSR 0833–45. Double pulses were detected from an area which included Lasker's1 star M. The pulsed emission has a time-averaged blue magnitude of approximately 25.2 min.

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References

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    Lasker, B. M. Astrophys. J. 203, 193–195 (1976).

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    Lasker, B. M., Bracker, S. B. & Saá, O. Astrophys. J. Lett. 176, L65–L68 (1972).

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Author information

Affiliations

  1. Anglo-Australian Observatory, P.O. Box 296, Epping, NSW, 2121, Australia

    • P. T. WALLACE
    • , B. A. PETERSON
    • , P. G. MURDIN
    •  & I. J. DANZIGER
  2. CSIRO Division of Radiophysics, P.O. Box 76, Epping, NSW, 2121, Australia

    • R. N. MANCHESTER
    • , A. G. LYNE
    •  & W. M. Goss
  3. Royal Greenwich Observatory, Hailsham, East Sussex, UK

    • F. G. SMITH
    • , M. J. DISNEY
    • , K. F. HARTLEY
    • , D. H. P. JONES
    •  & G. W. WELLGATE

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https://doi.org/10.1038/266692a0

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