The Distributions of Apparent Beamwidth for the Sheet-Shape Radiation Beam of Pulsars

Details The Distributions of Apparent Beamwidth for the Sheet-Shape Radiation Beam of Pulsars The Distributions of Apparent Beamwidth for the Sheet-Shape Radiation Beam of Pulsars

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983acaps...3....9q&link_type=abstract

Acta Astrophysica Sinica, Vol. 3, P. 15, 1983

Astronomy and Astrophysics

Astrophysics

Scientific paper

This paper is an extension of earlier work on a pulsar model, where the observed radio radiation is assumed to originate in the regions close to the magnetic equator of a neutron star and the radiation beam is in the shape of a sheet-like ring structure (sheet-shape radiation beam model). The equation describing the distribution of apparent beamwidths for this model is derived and integrated numerically. A comparison of the results with observed apparent beamwidths for a large sample of pulsars shows good agreement.

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