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Timing Observations of the SMC Binary PSR J0045-7319

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dc.contributor.author Kaspi, V. en_US
dc.contributor.author Manchester, R. en_US
dc.contributor.author Bailes, M. en_US
dc.contributor.author Bell, J. en_US
dc.date.accessioned 2004-10-05T06:35:43Z
dc.date.available 2004-10-05T06:35:43Z
dc.date.issued 1994-08 en_US
dc.identifier.citation The Hague, The Netherlands en_US
dc.identifier.clearanceno 94-1576 en_US
dc.identifier.uri http://hdl.handle.net/2014/33600
dc.description.abstract We describe radio timing observations of the binary pulsar PSR J0045-7319 made over the past 3.3 yr. We show that a simple timing model involving a standard Keplerian orbit well-describes the data, however significant low-level systematic residuals never before seen in other binary pulsars remain. We consider various possible origins of the residuals. en_US
dc.format.extent 440997 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other radio timing of pulsars radio timing of binary pulsars binary pulsar PSR J0045-7319 en_US
dc.title Timing Observations of the SMC Binary PSR J0045-7319 en_US


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