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19 April 2024
 
  » arxiv » 1204.5903

 Article overview


The XMM-Newton survey of the Small Magellanic Cloud: XMMUJ010633.1-731543 and XMMUJ010743.1-715953, two new Be/X-ray binary systems
M.J. Coe ; F. Haberl ; R. Sturm ; E.S. Bartlett ; D. Hatzidimitriou ; L.J. Townsend ; A. Udalski ; S. Mereghetti ; M. Filipovic ;
Date 26 Apr 2012
AbstractIn the course of the XMM-Newton survey of the Small Magellanic Cloud (SMC), two new bright X-ray sources were discovered exhibiting the spectral characteris- tics of High Mass X-ray Binaries - but revealing only weak evidence for pulsations in just one of the objects(at 153s in XMMUJ010743.1-715953). The accurate X- ray source locations permit the identi?cation of these X-ray source with Be stars, thereby strongly suggesting these systems are new Be/X-ray binaries. From blue spectra the proposed classi?cation for XMMUJ010633.1-731543 is B0.5-1Ve and for XMMUJ010743.1-715953 it is B2IV-Ve.
Source arXiv, 1204.5903
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