Abstract
A report of how rotating and oscillating magnetic neutron stars can account for the radio and optical signals from pulsars. Several predictions of the nature of the signals are put forward.
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References
Chiu, H.-Y., and Canuto, V., Phys. Rev. Lett., (in the press).
Canuto, V., Chiu, H.-Y., and Fassio-Canuto, L., Phys. Rev. (in the press).
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CHIU, HY., CANUTO, V. & FASSIO-CANUTO, L. Nature of Radio and Optical Emissions from Pulsars. Nature 221, 529–531 (1969). https://doi.org/10.1038/221529a0
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DOI: https://doi.org/10.1038/221529a0
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