Spin-down of pulsars by the current - Comparison of theory with observations

Details Spin-down of pulsars by the current - Comparison of theory with observations Spin-down of pulsars by the current - Comparison of theory with observations

Jul 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984ap%26ss.102..301b&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 102, no. 2, July 1984, p. 301-326.

Astronomy and Astrophysics

Astrophysics

44

Pulsar Magnetospheres, Pulsars, Rotating Plasmas, Stellar Radiation, Stellar Rotation, Distribution Functions, Electron Plasma, Plasma Composition, Statistical Analysis, Stellar Evolution

Scientific paper

Observational data are analysed on the basis of pulsar magnetosphere theory and the Ruderman-Sutherland plasma generation mechanism. The results of the theory and experiments are shown to be in good agreement. The existence of a special group of long-lived, weakly-radiating fast (the period P ≅ 0.1 - 0.4 s) and superfast (P ⪉ 0.01) pulsars is predicted.

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