Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-06-25
Astronomy and Astrophysics
Astrophysics
Accepted by MNRAS
Scientific paper
10.1111/j.1365-2966.2004.08150.x
Three new X-ray pulsars have been detected in the Small Magellanic Cloud (SMC) and the positions of two others have been determined, with archive Chandra data. A series of five observations of the SMC took place between May and October 2002. Analysis of these data has revealed three previously unknown X-ray pulsars at pulse periods of 34, 503 and 138 seconds. The position of pulsar XTE J0052-725, which was originally detected by RXTE on June 19 2002, was also accurately determined and a previously detected 7.78s RXTE pulsar was identified as the source SMC X-3.
Coe Malcolm J.
Corbet Robin H. D.
Edge W. R. T.
Galache Jose Louis
Laycock Silas
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