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Search for Optical Flashes from the Radio Source CP 1919

  • J. V. Jelley
  • R. V. Willstrop

Abstract

The four rapidly pulsating radio sources discovered by Hewish et al. 1 have been tentatively identified with neutron stars or white dwarfs, and their optical identification is therefore of great interest.

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Referenzen

  1. 1.
    Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature, 217, 709 (1968), (Paper 1).ADSCrossRefGoogle Scholar
  2. 2.
    Ryle, M., and Bailey, J. A., Nature, 217, 907 (1968), (Paper 19).ADSCrossRefGoogle Scholar
  3. 3.
    Hewish, A., Meeting of the Royal Astronomical Society (London. April 10, 1968).Google Scholar
  4. 4.
    Johnson, H. L., Astrophys. J., 116, 640 (1952).ADSCrossRefGoogle Scholar
  5. 5.
    Davies, J. G., Horton, P. W., Lyne, A. G., Rickett, B. J., and Smith, F. G., Nature, 217, 910 (1968), (Paper 6).ADSCrossRefGoogle Scholar
  6. 6.
    Radhakrishnan, V., Komesaroff, M. M., and Cooke, D. J., Nature, 218, 229 (1968), (Paper 17).ADSCrossRefGoogle Scholar

Copyright information

© Springer Science+Business Media New York 1968

Authors and Affiliations

  • J. V. Jelley
    • 1
  • R. V. Willstrop
    • 2
  1. 1.Aere, HarwellUK
  2. 2.University of CambridgeObservatoriesUSA

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