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Glitches in Southern Pulsars

Published online by Cambridge University Press:  12 April 2016

Na Wang
Affiliation:
Urumqi Astronomical Observatory, 40 South Beijing Road, Urumqi 830011, China
R. N. Manchester
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping NSW 1710, Australia
R. Pace
Affiliation:
Australia Telescope National Facility, CSIRO, PO Box 76, Epping NSW 1710, Australia
M. Bailes
Affiliation:
Astrophysics and Supercomputing, Swinburne University of Technolgy, PO Box 218, Hawthorn Vic. 3122, Australia
V. M. Kaspi
Affiliation:
MIT, Center for Space Research 37-621, 70 Vassar St., Cambridge MA 02139, USA
B.W. Stappers
Affiliation:
Mt Stromlo Observatory, ANU, Private Bag, Weston Creek ACT 2611, Australia
A. G. Lyne
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK

Abstract

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Parkes timing observations of 31 mostly young pulsars over nearly nine years are described. A total of 29 glitches were detected, of which 19 are previously unreported. Twelve glitches were seen in PSR J1341–6220, making this the most frequently glitching pulsar known, and the largest known glitch was detected in PSR J1614–5047. Distributions of glitch parameters were investigated.

Type
Part 2. Timing, General Relativity and Astrometry
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Shemar, S.L. & Lyne, A.G. 1996, MNRAS, 282, 677 Google Scholar
Wang, N., Manchester, R.N., Pace, R., Bailes, M., Kaspi, V.M., Stappers, B.W. & Lyne, A.G. 1999, MNRAS, submitted.Google Scholar