Abstract
Neutron stars may support torsional oscillations, having periods in the lowest mode of a few tenths of a second, similar to the periods of the pulsed radio sources.
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RUDERMAN, M. Crystallization and Torsional Oscillations of Superdense Stars. Nature 218, 1128–1129 (1968). https://doi.org/10.1038/2181128a0
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DOI: https://doi.org/10.1038/2181128a0
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