Lyne, A. G. and Brinklow, A. and Middleditch, J. and Kulkarni, S. R. and Backer, D. C. and Clifton, T. R. (1987) The discovery of a millisecond pulsar in the globular cluster M28. Nature, 328 (6129). pp. 399-401. ISSN 0028-0836. doi:10.1038/328399a0. https://resolver.caltech.edu/CaltechAUTHORS:20131126-151331718
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Abstract
Here we report the discovery of a pulsar with a 3 millisecond period in the core of the globular cluster M28. The existence of a millisecond pulsar in such a cluster, where there are frequent interactions between cluster stars, provides strong confirmation of the theory that the high rotation rate derives from accretion in a binary system. The pulsar is now isolated, having no binary companion.
Item Type: | Article | |||||||||
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Additional Information: | © 1987 Nature Publishing Group. Received 24 June; accepted 2 July 1987. | |||||||||
Group: | UNSPECIFIED, Division of Geological and Planetary Sciences | |||||||||
Issue or Number: | 6129 | |||||||||
DOI: | 10.1038/328399a0 | |||||||||
Record Number: | CaltechAUTHORS:20131126-151331718 | |||||||||
Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20131126-151331718 | |||||||||
Official Citation: | The discovery of a millisecond pulsar in the globular cluster M28 399 A.G. Lyne, A. Brinklow, J. Middleditch, S.R. Kulkarni, D.C. Backer & T.R. Clifton | |||||||||
Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
ID Code: | 42743 | |||||||||
Collection: | CaltechAUTHORS | |||||||||
Deposited By: | Ruth Sustaita | |||||||||
Deposited On: | 27 Nov 2013 16:41 | |||||||||
Last Modified: | 10 Nov 2021 16:27 |
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