Abstract
New observations make a binary star model unlikely and reveal complex frequency structure in individual pulses.
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References
Hewish, A., Bell, S. J., Pilkington, J. D. H., Scott, P. F., and Collins, R. A., Nature, 217, 709 (1968).
Pilkington, J. D. H., Hewish, A., Bell, S. J., and Cole, T. W., Nature, 218, 126 (1968).
Saslaw, W. C., Faulkner, J., and Strittmatter, P. A., Nature, 217, 1222 (1968).
Ostriker, J., Nature, 217, 1227 (1968).
Ryle, M., J. Inst. Elect. Eng., 6, 14 (1960).
Davies, J. G., Horton, P. W., Lyne, A. G., Rickett, B. J., and Smith, F. G., Nature, 217, 910 (1968).
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SCOTT, P., COLLINS, R. Further Observations of Pulsating Radio Sources. Nature 218, 230–232 (1968). https://doi.org/10.1038/218230a0
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DOI: https://doi.org/10.1038/218230a0
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