High energy electrons in pulsar magnetospheres

Details High energy electrons in pulsar magnetospheres High energy electrons in pulsar magnetospheres

Apr 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982mnras.199..211d&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 199, Apr. 1982, p. 211-217. Research supported by the Science and Engin

Astronomy and Astrophysics

Astronomy

20

High Energy Electrons, Pulsar Magnetospheres, Pulsars, Stellar Atmospheres, Stellar Radiation, Electron Trajectories, Gamma Ray Astronomy, Stellar Magnetic Fields

Scientific paper

Magnetospheres of pulsars contain charged particles. The motion of electrons and positrons in a simplified cylindrical model is discussed for a pulsar with the period of the Crab. It will be shown that this motion near the light cylinder provides a mechanism for the production of incoherent radiation at gamma ray frequencies. Such radiation has been observed in the Crab and the Vela pulsars.

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