Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-26T04:37:36.143Z Has data issue: false hasContentIssue false
  • English
  • Français

A Large Timing Discontinuity in the Vela Pulsar, July 1985

Published online by Cambridge University Press:  04 August 2017

C S Flanagan
C S Flanagan*
Affiliation:
National Institute for Telecommunications Research, CSIR. P O Box 3718, Johannesburg, South Africa

Extract

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.

A pulsar-monitoring programme has been running at Hartebeesthoek Radio Astronomy Observatory over the last three years, at 2.32 and (during the last year) at 1.67 GHz. Twenty pulsars are observed once or twice a fortnight, and PSRs 1641-45 and 0833-45 (the Vela pulsar) daily.

Type
I. Rotation-Powered Pulsars
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 64
Copyright
Copyright © Reidel 1987