Abstract
A model for pulsars based on vibrating white dwarf stars accounts for a number of the features of the emissions, and also gives rise to the possibility of optical fluctuations having a period twice that of the radio pulses.
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CCCKE, W., COHEN, J. Pulsar Models. Nature 219, 1009–1012 (1968). https://doi.org/10.1038/2191009a0
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DOI: https://doi.org/10.1038/2191009a0
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