Publication Abstracts

Hansen 1966

Hansen, C.J., 1966: Neutrino energy losses from vibrating neutron stars. Nature, 211, no. 5053, 1069-1070, doi:10.1038/2111069a0.

It has been suggested by Cameron that the spectra of discrete X-ray sources in the sky may arise from two sources, each attributable to the presence of neutron stars: a thermal component emitted from the photosphere of the star and a non-thermal synchrotron or bremsstrahlung component emitted by electrons accelerated in a vibrating magnetosphere. It is assumed that the latter process derives its energy from stored gravitational energy in the form of radial oscillations with characteristic fundamental frequencies in the 103 c/s range.

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BibTeX Citation

@article{ha00120c,
  author={Hansen, C. J.},
  title={Neutrino energy losses from vibrating neutron stars},
  year={1966},
  journal={Nature},
  volume={211},
  number={5053},
  pages={1069--1070},
  doi={10.1038/2111069a0},
}

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RIS Citation

TY  - JOUR
ID  - ha00120c
AU  - Hansen, C. J.
PY  - 1966
TI  - Neutrino energy losses from vibrating neutron stars
JA  - Nature
JO  - Nature
VL  - 211
IS  - 5053
SP  - 1069
EP  - 1070
DO  - 10.1038/2111069a0
ER  -

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