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In the course of the  XMM–Newton  survey of the Small Magellanic Cloud (SMC), two new bright X‐ray sources were discovered exhibiting the spectral characteristics of high‐mass X‐ray binaries – but revealing only weak evidence for pulsations in just one of the objects (at 153 s in XMMU J010743.1−715953). The accurate X‐ray source locations permit the identification of these X‐ray sources with Be stars, thereby strongly suggesting that these systems are new Be/X‐ray binaries. From blue spectra the proposed classification for XMMU J010633.1−731543 is B0.5‐1Ve and for XMMU J010743.1−715953 it is B2IV‐Ve.

The XMM–Newton survey of the Small Magellanic Cloud: XMMU J010633.1−731543 and XMMU J010743.1−715953, two new Be/X‐ray binary systems ★