Abstract
OBSERVATIONS with the Parkes 210 foot telescope during May and June 1968 have shown spectral features in the 150 MHz emission from pulsars with bandwidths as narrow as 0.5 MHz. The sources observed were CP 1919, CP 0950 and CP 1133.
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References
Robinson, B. J., Wielbinski, R., Cooper, B. F. C., and Landecker, T. L., Nature, 218, 1143 (1968).
Lyne, A. G., and Rickett, B. J., Nature, 218, 326 (1968).
Scheuer, P. A. G., Nature, 218, 920 (1968).
Slee, O. B., Komesaroff, M. M., and McCulloch, P. M., Nature, 219, 342 (1968).
Scott, P. F., and Collins, R. A., Nature, 218, 230 (1968).
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KOMESAROFF, M., MCCULLOCH, P., HAMILTON, P. et al. Spectral Fine Structure in Pulsar Radiation. Nature 220, 358–360 (1968). https://doi.org/10.1038/220358a0
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DOI: https://doi.org/10.1038/220358a0
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