Pulsar electrodynamics - Cylindrical model and radio and gamma-ray radiation

Details Pulsar electrodynamics - Cylindrical model and radio and gamma-ray radiation Pulsar electrodynamics - Cylindrical model and radio and gamma-ray radiation

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.204.1125d&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 204, Sept. 1983, p. 1125-1144. Research supported by th

Astronomy and Astrophysics

Astronomy

11

Electrodynamics, Gamma Ray Astronomy, Pulsar Magnetospheres, Pulsars, Radio Astronomy, Stellar Models, Equations Of Motion, Particle Motion, Stellar Radiation

Scientific paper

Magnetospheres of pulsars contain charged particles. The motion of electrons and positrons in a simplified cylindrical model is discussed for pulsars with three different periods. It will be shown that this motion near the region E = cB provides not only a mechanism for the production of incoherent radiation at gamma-ray frequencies but also the basis to explain the radio emission. A single region to explain the radiation in both frequency domains is supported by observations of the Crab Pulsar.

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