Publication Abstracts
Chiu and Canuto 1969
Chiu, H.-Y., and
, 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={Physical Review Letters}, 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. JO - Physical Review Letters VL - 22 SP - 415 EP - 419 DO - 10.1103/PhysRevLett.22.415 ER -
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