@article {23862,
	title = {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<SUP>*</SUP>},
	volume = {424},
	year = {2012},
	month = {2012/07/1},
	pages = {282 - 292},
	abstract = {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.},
	keywords = {Astrophysics - High Energy Astrophysical Phenomena, stars: neutron, X-rays: binaries},
	isbn = {0035-8711},
	url = {https://ui.adsabs.harvard.edu/abs/2012MNRAS.424..282C},
	author = {Coe, M. J. and Haberl, F. and Sturm, R. and Bartlett, E. S. and Hatzidimitriou, D. and Townsend, L. J. and Udalski, A. and Mereghetti, S. and Filipovi{\'c}, M.}
}
