Phys. Rev. Lett. 34, 901–905 (1975)Synchrotron Emission from an Oblique Rotator and Its Application to PulsarsReceived 24 June 1974; published in the issue dated 7 April 1975 A method is presented which permits rapid interpretation of the synchrotron patterns emitted by a charged particle moving in the uniform magnetic field of an oblique rotator. The analysis predicts a variety of intensity and polarization patterns that are compared with data from a number of pulsars. It also predicts the observed frequency dependence of the peak-to-peak separation of two double-peaked pulsars. © 1975 The American Physical Society URL:
http://link.aps.org/doi/10.1103/PhysRevLett.34.901
DOI:
10.1103/PhysRevLett.34.901
PACS:
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