Cohen and Cameron 1969
Cohen, J.M., and A.G.W. Cameron, 1969: Rotational properties of neutron star models. Nature, 224, 566-567, doi:10.1038/224566a0.
It has been suggested that pulsars are rotating neutron stars and that the energy source of the Crab nebula is the loss of rotational energy from the Crab pulsar. Because neutron stars are quite dense, general relativistic effects are large and cannot be neglected.
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Cohen, J.M., and Cameron, A.G.W.: Rotational properties of neutron star models, Nature, 224, 566-567, doi:10.1038/224566a0, 1969.
Cohen, J.M., and A.G.W. Cameron (1969), Rotational properties of neutron star models, Nature, 224, 566-567, doi:10.1038/224566a0.
Cohen, J.M., and A.G.W. Cameron, 1969: Rotational properties of neutron star models. Nature, 224, 566-567, doi:10.1038/224566a0.
Cohen, J.M., & Cameron, A.G.W. 1969, Nature, 224, 566, doi:10.1038/224566a0.
Cohen JM, Cameron AGW. Rotational properties of neutron star models, Nature 1969;224:566-567. doi:10.1038/224566a0.
J.M. Cohen, A.G.W. Cameron, Nature 224, 566-567, doi:10.1038/224566a0 (1969).
