Hostname: page-component-6bf8c574d5-gr6zb Total loading time: 0 Render date: 2025-02-23T13:59:12.617Z Has data issue: false hasContentIssue false
  • English
  • Français

Long-term Radio Timing Observations of PSR B1509–58

Published online by Cambridge University Press:  19 July 2016

Margaret A. Livingstone ,
Victoria M. Kaspi  and
Richard N. Manchester
Margaret A. Livingstone
Affiliation:
McGill University, 3600 University Ave, Montreal, Quebec, H3A 2T8, Canada
Victoria M. Kaspi
Affiliation:
McGill University, 3600 University Ave, Montreal, Quebec, H3A 2T8, Canada
Richard N. Manchester
Affiliation:
Australia Telescope National Facility, CSIRO, P.O. Box 76, Epping NSW 1710, Australia

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.

We present an updated phase-coherent timing solution for the young, energetic pulsar B1509–58 from twenty years of data. Using a partially phase-coherent timing analysis, we show that the second frequency derivative is changing in time, implying a third frequency derivative of This value is consistent with the simple power law model of pulsar rotation.

Type
Part 10: Radio Pulsar Timing
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 425 - 426
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Kaspi, V. M., Manchester, R. N., Siegman, B., Johnston, S., & Lyne, A. G. 1994, ApJ, 422, L83.CrossRefGoogle Scholar
Manchester, R. N., & Taylor, J. H. 1977, Pulsars, (San Francisco: Freeman)Google Scholar