Statistical study of the pulse width distribution for radio pulsars

Details Statistical study of the pulse width distribution for radio pulsars Statistical study of the pulse width distribution for radio pulsars

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010scchg..53s.220c&link_type=abstract

Science China Physics, Mechanics and Astronomy, Volume 53, Issue 1, pp.220-223

Astronomy and Astrophysics

Astronomy

Pulsar, Pulse Width, Emission Beam, Random Distribution

Scientific paper

Pulse widths of standard pulse profiles for 262 pulsars were measured by using the Urumqi 25 m radio telescope at 1.54 GHz. For the simplest case of circular emission beam, we applied Monte Carlo simulations to the pulse width distribution. Different density functions of magnetic inclination angle α and observer angle ζ were considered. Using Kolmogorov-Smirnov tests, we derived the most probable distribution for α and ζ.

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