Publication Abstracts

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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BibTeX Citation

@article{co00200p,
  author={Cohen, J. M. and Cameron, A. G. W.},
  title={Rotational properties of neutron star models},
  year={1969},
  journal={Nature},
  volume={224},
  pages={566--567},
  doi={10.1038/224566a0},
}

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RIS Citation

TY  - JOUR
ID  - co00200p
AU  - Cohen, J. M.
AU  - Cameron, A. G. W.
PY  - 1969
TI  - Rotational properties of neutron star models
JA  - Nature
VL  - 224
SP  - 566
EP  - 567
DO  - 10.1038/224566a0
ER  -

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