Hostname: page-component-8448b6f56d-c47g7 Total loading time: 0 Render date: 2024-04-24T05:14:42.073Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

Gold, T.: 1969, Nature 221, 25.Google Scholar
Goldreich, P. and Julian, W.: 1969, Astrophys. J. 157, 869.Google Scholar
Ostriker, J. P. and Gunn, J.: 1969, Astrophys. J. 157, 1395.CrossRefGoogle Scholar
Pollack, J. B. and Shen, B. S. P.: 1969, Phys. Rev. Letters 23, 1358.Google Scholar