Hostname: page-component-7bb8b95d7b-5mhkq Total loading time: 0 Render date: 2024-09-28T21:25:03.887Z Has data issue: false hasContentIssue false
  • English
  • Français

The Comparative Properties of the Pulsars

Published online by Cambridge University Press:  07 February 2017

A. G. Lyne
A. G. Lyne*
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, U.K.

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.

This paper reviews the outstanding characteristics of the pulsars and, in particular, compares the properties of the Crab Nebula pulsar with those of the other pulsars. The Crab pulsar is unique in that it has a remarkably short period, emission outside the radio band, some strange amplitude variations and an abnormally large interpulse.

Type
Session 3
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 182 - 194
Copyright
Copyright © Reidel 1971 

References

Cole, T. W., Hesse, H. K., and Page, C. G.: 1970, Nature 225, 712.CrossRefGoogle Scholar
Craft, H. D. and Comella, J. M.: 1968, Nature 220, 676.CrossRefGoogle Scholar
Drake, F. D. and Craft, H. D.: 1968, Nature 220, 231.CrossRefGoogle Scholar
Hunt, G. C.: 1969, Nature 224, 1005.CrossRefGoogle Scholar
Radhakrishnan, V. and Manchester, R. N.: 1969, Nature 222, 228.CrossRefGoogle Scholar
Reichley, P. E. and Downs, G. S.: 1969, Nature 222, 229.CrossRefGoogle Scholar
Reichley, P. E., Downs, G. S., and Morris, G. A.: 1970, Astrophys. J. 159, L35.CrossRefGoogle Scholar