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Thirteen Drift Bands in PSR B0826–34

Published online by Cambridge University Press:  19 July 2016

A. Esamdin ,
A. G. Lyne ,
M. Kramer ,
F. Graham-Smith  and
R. N. Manchester
A. Esamdin
Affiliation:
National Astronomical Observatories/Urumqi Observatory, CAS Urumqi 830011, P. R. China
A. G. Lyne
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
M. Kramer
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
F. Graham-Smith
Affiliation:
University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, UK
R. N. Manchester
Affiliation:
Australia Telescope National Facility, CSIRO, P. O. Box 76, Epping NSW 1710, Australia

Abstract

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By developing a new technique, 13 drifting subpulses have been revealed across one period in PSR B0826–34. The variation of drift rate when drifting subpulses drift through different longitude regions are noticed. A weak emission mode was detected during its apparent null.

Type
Part 7: Observations of Pulsed Emission
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 341 - 342
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Biggs, J. D., McCulloch, P. M., Hamilton, P. A., Manchester, R. N., & Lyne, A. G. 1985, MNRAS, 215, 281.CrossRefGoogle Scholar
Durdin, J. M., Large, M. I., Little, A. G., Manchester, R. N., Lyne, A. G., & Taylor, J. H. 1979, MNRAS, 186, 39P.Google Scholar