Publication Abstracts

Chiu and Canuto 1969

Chiu, H.-Y., and V. Canuto, 1969: Radio emission from magnetic neutron stars. A possible model for pulsars. Phys. Rev. Lett., 22, 415-419, doi:10.1103/PhysRevLett.22.415.

We show that radio emission from a neutron star with a magnetic field of 109 G or more can account for the radio emission of pulsars. It is suggested that pulsars also emit two bands, one in the uv or optical, and the other in the infrared in the decamicron wavelength range.

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BibTeX Citation

@article{ch09100s,
  author={Chiu, H.-Y. and Canuto, V.},
  title={Radio emission from magnetic neutron stars. A possible model for pulsars},
  year={1969},
  journal={Phys. Rev. Lett.},
  volume={22},
  pages={415--419},
  doi={10.1103/PhysRevLett.22.415},
}

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RIS Citation

TY  - JOUR
ID  - ch09100s
AU  - Chiu, H.-Y.
AU  - Canuto, V.
PY  - 1969
TI  - Radio emission from magnetic neutron stars. A possible model for pulsars
JA  - Phys. Rev. Lett.
VL  - 22
SP  - 415
EP  - 419
DO  - 10.1103/PhysRevLett.22.415
ER  -

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