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25 April 2024
 
  » arxiv » 1103.0195

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The XMM-Newton survey of the Small Magellanic Cloud: XMMUJ005011.2-730026 = SXP214, a Be/X-ray binary pulsar
M. J. Coe ; F. Haberl ; R. Sturm ; W. Pietsch ; L.J. Townsend ; E.S. Bartlett ; M. Filipovic ; A. Udalski ; R.H.D. Corbet ; A. Tiengo ; M. Ehle ; J.L. Payne ; D. Burton ;
Date 1 Mar 2011
AbstractIn the course of the XMM-Newton survey of the Small Magellanic Cloud (SMC), a region to the east of the emission nebula N19 was observed in November 2009. To search for new candidates for high mass X-ray binaries the EPIC PN and MOS data of the detected point sources were investigated and their spectral and temporal characteristics identified. A new transient (XMMUJ005011.2-730026= SXP214) with a pulse period of 214.05 s was discovered; the source had a hard X-ray spectrum with power-law index of ~0.65. The accurate X-ray source location permits the identification of the X-ray source with a ~15th magnitude Be star, thereby confirming this system as a new Be/X-ray binary.
Source arXiv, 1103.0195
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