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In this paper we have used the data of 1315 pulsars (Guseinov et al., 2002) for statistical analysis and showed the changes in pulsar parameters since the appearance of Taylor et al. (1996) catalog. Here we present the space distribution of pulsars, dispersion measures, distances from the galactic plane and from the Sun, electron density, luminosity distributions at 400 and $1400\,\hbox{MHz}$, the relations between luminosities of pulsars at 400 and $1400\,\hbox{MHz}$ and the dependence of luminosity on age and on magnetic field. We also present the updated $P\ndash \dot{P}$ diagram.
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Keywords: Compact stars; Neutron stars; Pulsars

Document Type: Research Article

Affiliations: 1: Department of Physics, Middle East Technical University, Ankara, Turkey 2: Department of Physics, Akdeniz University, Antalya, Turkey 3: Physics Institute, Academy of Science, Baku 370143, Azerbaijan Republic

Publication date: 01 June 2003

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