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Observational Properties of Pulsars

  • Edward J. Groth
Part of the Astrophysics and Space Science Library book series (ASSL, volume 48)

Abstract

In the six years since the announcement [129] of the discovery of the first pulsar, a total of 105 pulsars have been discovered and a great deal has been learned of their properties. Pulsars are slowly rotating (~1 Hz) neutron stars with huge magnetic fields (~1012 G) which convert rotational energy into energy of (radio) radiation and relativistic particles. The pulsed radiation presumably arises from a beaming effect associated with the magnetic field.

Keywords

Neutron Star Spectral Index Faraday Rotation Supernova Remnant Dispersion Measure 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company, Dordrecht-Holland 1975

Authors and Affiliations

  • Edward J. Groth
    • 1
  1. 1.Joseph Henry Laboratories, Physics Dept.Princeton UniversityPrincetonUSA

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