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Accurate Positions of CP 0950 and CP 1133

  • C. D. Mackay
  • B. Elsmore
  • J. A. Bailey

Abstract

Further observations with the one mile radio telescope1 have recently been made in order to improve the accuracy of the positions of the four pulsed radio sources reported by Hewish et al. 2.

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Referenzen

  1. 1.
    Elsmore, B., Kenderdine, S., and Ryle, M., Mon. Not. Roy. Astro. Soc., 134, 87 (1966).ADSGoogle Scholar
  2. 2.
    Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature. 217, 709 (1968), (Paper 1).ADSCrossRefGoogle Scholar
  3. 3.
    Ryle, M., and Bailey, J. A., Nature, 217, 907 (1968), (Paper 19).ADSCrossRefGoogle Scholar
  4. 4.
    Bailey, J. A., and Mackay, C. D., Nature, 218, 129 (1968), (Paper 20).ADSCrossRefGoogle Scholar
  5. 5.
    Pilkington, J. D. H., Hewish, A., Bell, S. J., and Cole, T. W., Nature, 218, 126 (1968), (Paper 2).ADSCrossRefGoogle Scholar
  6. 6.
    Lyne, A. G., and Rickett, B. J., Nature, 218, 326 (1968), (Paper 10).ADSCrossRefGoogle Scholar
  7. 7.
    Allen, C. W., Astrophysical Quantities (Athlone Press, 1963).Google Scholar

Copyright information

© Springer Science+Business Media New York 1968

Authors and Affiliations

  • C. D. Mackay
    • 1
  • B. Elsmore
    • 1
  • J. A. Bailey
    • 1
  1. 1.Mullard Radio Astronomy Observatory, Cavendish LaboratoryUniversity of CambridgeUK

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