On the pulse-width statistics in radio pulsars
Institute of Nuclear Physics, Radzikowskiego 152, 31-342 Kraków, Poland
2 Institute of Astronomy, Jagiellonian University, Orla 171, 30-244 Kraków, Poland
3 Institute of Astronomy, University of Zielona Góra, Lubuska 2, 65-265 Zielona Góra, Poland e-mail: firstname.lastname@example.org
Accepted: 28 July 2004
We perform Monte Carlo simulations of pulsar periods, pulse-widths and magnetic inclination angles. Using the available observational data sets we study possible parent distribution functions by means of the Kolmogorov-Smirnov significance tests. We also use an additional condition that the numbers of generated interpulses, whether from both magnetic poles or from a single pole, are at the observed levels. We derived a model distribution function of magnetic inclination angles which has a local maximum near and another weaker one near . The gamma function is a plausible distribution function describing pulsar periods. The average beaming fraction describing the fraction of observable radio pulsars is about 0.12.
Key words: stars: pulsars: general / stars: neutron / stars: rotation
© ESO, 2004