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
Elsmore, B., Kenderdine, S., and Ryle, M., Mon. Not. Roy. Astro. Soc., 134, 87 (1966).
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature. 217, 709 (1968), (Paper 1).
Ryle, M., and Bailey, J. A., Nature, 217, 907 (1968), (Paper 19).
Bailey, J. A., and Mackay, C. D., Nature, 218, 129 (1968), (Paper 20).
Pilkington, J. D. H., Hewish, A., Bell, S. J., and Cole, T. W., Nature, 218, 126 (1968), (Paper 2).
Lyne, A. G., and Rickett, B. J., Nature, 218, 326 (1968), (Paper 10).
Allen, C. W., Astrophysical Quantities (Athlone Press, 1963).
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Mackay, C.D., Elsmore, B., Bailey, J.A. (1968). Accurate Positions of CP 0950 and CP 1133. In: Pulsating Stars. Springer, Boston, MA. https://doi.org/10.1007/978-1-4899-6387-1_21
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DOI: https://doi.org/10.1007/978-1-4899-6387-1_21
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