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A New Look at the Classification of Pulsars

Published online by Cambridge University Press:  27 September 2017

Igor F. Malov
Igor F. Malov*
Affiliation:
Radio Astronomy Department, Lebedev Physical Institute

Abstract

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It is shown that pulsars with long periods differ systematically from those with short periods. We conclude that generation of emission in the second group occurs in a very thin layer (near the light cylinder). Relativistic effects may be significant here. Some properties of core emission can be explained by Melrose's mechanism.

Type
Part III Magnetospheric models
Information
International Astronomical Union Colloquium , Volume 128: Magnetospheric structure and emission mechanisms of radio pulsars , 1992 , pp. 103 - 104
Copyright
Copyright © United States Naval Observatory 1992