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Secondary Periodicities in Four Strong Pulsars at 80 MHz

Published online by Cambridge University Press:  25 April 2016

O. B. Slee
Affiliation:
Division of Radiophysics, CSIRO, Sydney
P. S. Mulhall
Affiliation:
Division of Radiophysics, CSIRO, Sydney

Extract

During the interval May 1968 to March 1969 the 80 MHz radioheliograph at Culgoora has been used in a detailed study of the intensity variations in the pulsars CP 0834, 0950, 1133 and 1919. Some preliminary results for CP 1133 and 1919 have already been reported.

Type
Contributions
Copyright
Copyright © Astronomical Society of Australia 1970

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References

1 Slee, O. B., Proc ASA, 1, 223 (1969).Google Scholar
2 Cooley, J. W. and Tukey, J. W., Math. Comput., 19, 297 (1965).CrossRefGoogle Scholar
3 Bingham, C., Godfrey, M. D. and Tukey, J. W., IEEE Trans., AU-15, 56 (1967).Google Scholar
4 Taylor, J. H., Jura, M. and Huguenin, G. R., Nature, 223, 797 (1969).CrossRefGoogle Scholar
5 Conklin, E. K., Howard, H. T., Craft, H. D. and Cornelia, J. M., Nature, 219, 1238 (1968).CrossRefGoogle Scholar
6 Lovelace, R. V. E. and Craft, H. D., Nature, 220, 875 (1968).CrossRefGoogle Scholar
7 Drake, F. D. and Craft, H. D., Nature, 220, 231 (1968).CrossRefGoogle Scholar