Distances and Other Parameters for 1315 Radio Pulsar

Abstract

In this work we have collected observational data for 1315 PSRs. Distances and others parameters for these PSRs were estimated. We present improved distance estimates for radio pulsars by considering importance of their physical properties and improvement of distribution of SFRs (star formation regions) in the Galaxy. For this purpose, both a list of accurate calibrators was constructed and several accurate criteria were established. The following values were calculated from PSRs observational data: luminosities at 400 Mhz and 1400 Mhz, characteristic times, strength of magnetic field and rate of rotation energy. This compilation of data is mainly necessary for statistical investigations and for the physical properties of neutron stars. The whole data is prepared in a publicly accessible web page: http://www.xrbc.org/pulsar/ .

8 pages, 1 figure, submitted to Astronomical Notices

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Cited by in corpus (5)

• Suzaku observation of the unidentified VHE gamma-ray source HESS J1702-420
• Effects of the background radiation on radio pulsar and supernova remnant searches and the birth rates of these objects
• Birth rates of different types of neutron star and possible evolutions of these objects
• Magnetospheric particle acceleration and X-ray emission of pulsars
• Pulsar Luminosity Function