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Young Pulsars – Pulsed Neutron Sources

Published online by Cambridge University Press:  07 February 2017

J. Truemper
J. Truemper*
Affiliation:
Max-Planck-Institut für Physik und Astrophysik, Institut für Extraterrestrische Physik, Garching b. München, Germany

Abstract

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The prospects of observing a pulsed neutron flux at very high energies from pulsars are discussed. Most likely candidates are the Vela pulsar at 2 × 1016 eV and the Crab Pulsar at 1017 eV.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 384 - 385
Copyright
Copyright © Reidel 1971 

References

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