Evolution of radiopulsars with consideration of their having originated in part in binaries

Details Evolution of radiopulsars with consideration of their having originated in part in binaries Evolution of radiopulsars with consideration of their having originated in part in binaries

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..512v&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, May-June 1991, p. 512-521. In Russian.

Astronomy and Astrophysics

Astronomy

Binary Stars, Pulsars, Radio Stars, Star Clusters, Stellar Evolution, Milky Way Galaxy, Radio Astronomy, Stellar Mass Accretion, Stellar Models

Scientific paper

The differences between two types of radiopulsars detected by 5D cluster analysis are studied. The foremost difference is that Crab-like pulsars exhibit smooth and monotonic changes in all observable parameters depending on their distance from the galactic plane z. The pulsars that probably passed the accretion stage in binaries have no such dependence for any of the parameters studied. The data obtained are in agreement with the evolution model in which some part of pulsars was formed in binaries.

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