Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-26T05:15:49.151Z Has data issue: false hasContentIssue false
  • English
  • Français

A Massive Glitch in PSR 0355+54

Published online by Cambridge University Press:  04 August 2017

A.G. Lyne
A.G. Lyne*
Affiliation:
University of Manchester, Nuffield Radio Astronomy Laboratories, Jodrell Bank, Macclesfield Cheshire SK11 9DL, United Kingdom

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.

Pulse timing observations at Jodrell Bank have shown that the relatively old pulsar PSR 0355+54 has suffered two glitches in the last 18 months, the second glitch being larger than any previously observed in any pulsar.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 63
Copyright
Copyright © Reidel 1987 

References

Cordes, J.M. and Downs, G.S., 1985, Astrophys. J. Suppl., 59, 343.CrossRefGoogle Scholar
Pines, D. and Alpar, M.A., 1985. Nature, 316, 27.CrossRefGoogle Scholar