Pulsed high-energy radiation from oblique magnetic rotators

Details Pulsed high-energy radiation from oblique magnetic rotators Pulsed high-energy radiation from oblique magnetic rotators

Mar 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975ap%26ss..33..111f&link_type=abstract

Astrophysics and Space Science, vol. 33, Mar. 1975, p. 111-126. Consiglio Nazionale delle Ricerche

Astronomy and Astrophysics

Astrophysics

11

Electromagnetic Interactions, Particle Trajectories, Pulsars, Stellar Magnetic Fields, Stellar Rotation, Astronomical Models, Compton Effect, Dynamo Theory, Electromagnetic Fields, Emission Spectra, Energy Spectra, Equations Of Motion, Particle Acceleration, Pulsed Radiation

Scientific paper

A detailed analysis is reported of charged particle motion in the e.m. fields generated by oblique magnetic rotators. A full treatment of particle trajectories, radiated power and spectrum is given; astrophysical implications of these results in connection with pulsars, mainly NP 0532, are discussed and the possibility of a high energy pulsed radiation model with synchro-Compton emission at the speed-of-light cylinder is investigated.

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