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Millisecond Pulsars in 47 Tucanae

Published online by Cambridge University Press:  12 April 2016

Paulo C. Freire ,
Fernando Camilo ,
Duncan R. Lorimer ,
Andrew G. Lyne  and
Richard N. Manchester
Paulo C. Freire
Affiliation:
U. of Manchester, Jodrell Bank Observatory, Cheshire, SK11 9DL, UK
Fernando Camilo
Affiliation:
U. of Manchester, Jodrell Bank Observatory, Cheshire, SK11 9DL, UK
Duncan R. Lorimer
Affiliation:
NAIC, Arecibo Observatory, HC3 Box 53995, Arecibo, PR 00613, USA
Andrew G. Lyne
Affiliation:
U. of Manchester, Jodrell Bank Observatory, Cheshire, SK11 9DL, UK
Richard N. Manchester
Affiliation:
ATNF, CSIRO, P.O. Box 76, Epping NSW 1710, Australia

Abstract

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Recent observations of the globular cluster 47 Tuc, made with the Parkes telescope at a wavelength of 20 cm, have resulted in the discovery of nine new millisecond pulsars (MSPs), all in binary systems. The number of timing solutions available has risen from two to 14. These results will make possible a more detailed study of the cluster dynamics.

Type
Part 2. Timing, General Relativity and Astrometry
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 87 - 88
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Camilo, F., Lorimer, D.R., Freire, P., Lyne, A.G., Manchester, R.N. 2000, ApJ, in pressGoogle Scholar
Robinson, C.R., Lyne, A.G., Manchester, A.G., Bailes, M., D’Amico, N., & Johnston, S. 1995, MNRAS, 274, 547 CrossRefGoogle Scholar
Phinney, E.S. 1992, Philos. Trans. Roy. Soc. London A, 341, 39 Google Scholar