Synchrotron emission from an oblique rotator and its application to pulsars

Details Synchrotron emission from an oblique rotator and its application to pulsars Synchrotron emission from an oblique rotator and its application to pulsars

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975phrvl..34..901m&link_type=abstract

Physical Review Letters, vol. 34, Apr. 7, 1975, p. 901-905.

Astronomy and Astrophysics

Astrophysics

4

Astrophysics, Pulsars, Rotating Matter, Synchrotron Radiation, Charged Particles, Magnetic Fields, Polarization Characteristics

Scientific paper

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.

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