Evaluation of the angle between the magnetic and spin axes for 308 pulsars

Details Evaluation of the angle between the magnetic and spin axes for 308 pulsars Evaluation of the angle between the magnetic and spin axes for 308 pulsars

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..149k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Mar. 1983, p. 149-154) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Mar.-Apr.

Astronomy and Astrophysics

Astronomy

6

Pulsars, Radio Emission, Stellar Magnetic Fields, Stellar Rotation, Axes Of Rotation, Lorentz Force, Magnetic Field Configurations, Stellar Models

Scientific paper

The observed width of the integrated pulse profile of a pulsar will differ from the beamwidth of its radio emission, suggesting a method for determining the inclination beta of the magnetic axis to the rotation axis. The angle beta is evaluated for 308 pulsars, and is found to diminish as a pulsar grows older. Estimates are also obtained for the height of the emission region, and for the Lorentz factor gamma and number density of the radiating particles.

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