Spatial distribution of pulsars

Details Spatial distribution of pulsars Spatial distribution of pulsars

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61..708g&link_type=abstract

(Astronomicheskii Zhurnal, vol. 61, July-Aug. 1984, p. 708-726) Soviet Astronomy (ISSN 0038-5301), vol. 28, July-Aug. 1984, p. 4

Astronomy and Astrophysics

Astronomy

8

Astronomical Catalogs, Electron Density (Concentration), Pulsars, Spatial Distribution, Astrometry, Interstellar Matter, Longitude, Milky Way Galaxy

Scientific paper

A method for calculating electron density is used to determine the spatial distribution of the 331 known pulsars. The method takes into account a large amount of observational data for the physical characteristics of the interstellar medium; electron density increases in the Galaxy; and the dynamics of the pulsars themselves. The obtained pulsar distribution is given as a function of galactic longitude and distance from the sun. On the basis of the longitude and distance functions, some new physical parameters are calculated for the pulsars, and a complete list is given in a table.

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