Radio Emission From Magnetic Neutron Stars. A Possible Model for Pulsars

Details Radio Emission From Magnetic Neutron Stars. A Possible Model for Pulsars Radio Emission From Magnetic Neutron Stars. A Possible Model for Pulsars

Mar 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrvl..22..415c&link_type=abstract

Physical Review Letters, vol. 22, Issue 9, pp. 415-419

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21

Scientific paper

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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