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Microstructure and patterns of coherent radiation

Published online by Cambridge University Press:  12 April 2016

J. G. Ables  and
D. McConnell
J. G. Ables
Affiliation:
Div. of Radiophysics, CSIRO, PO Box 76, Epping 2121, Australia
D. McConnell
Affiliation:
Autralia Telescope National Facility, CSIRO, Locked Bag 194, Narrabri 2390, Australia

Abstract

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We present data which indicates that micropulses from the bright millisecond pulsar PSR J0437–4715 are observed at equally-spaced preferred phases within the pulse window. We find the pattern similar to that expected if each micropulse is radiated from a source with a coherence scale of ~ 100 m.

Type
Part 3 Radio Emission Processes
Information
International Astronomical Union Colloquium , Volume 160: Pulsars: Problems and Progress , 1996 , pp. 163 - 166
Copyright
Copyright © Astronomical Society of the Pacific 1996

References

Bell, J.F., Bailes, M., Manchester, R.N., Weisberg, J.M. & Lyne, A.G. 1995, ApJ, 440, L81 Google Scholar
Bracewell, R. 1965, “The Fourier Transform and its Applications”, McGraw-Hill, New York.Google Scholar
Hankins, T.H. 1971, ApJ, 169, 487 CrossRefGoogle Scholar
Lang, K.R. 1980, “Astrophysical Formulae”, Springer-Verlag, Germany.CrossRefGoogle Scholar
McConnell, D., Abies, J.G., Bailes, M. & Erickson, W.C. 1996, MNRAS, (In Press)Google Scholar