Radio Emission From Magnetic Neutron Stars. A Possible Model for Pulsars
- 3 March 1969
- journal article
- research article
- Published by American Physical Society (APS) in Physical Review Letters
- Vol. 22 (9), 415-419
- https://doi.org/10.1103/physrevlett.22.415
Abstract
We show that radio emission from a neutron star with a magnetic field of 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.
Keywords
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