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astro-ph.SR2026
SXP 31.0 -- the 2025 near-Eddington double X-ray outburst after 26 years of quiescence
Malcolm J. Coe, Thomas M. Gaudin, Itumeleng M. Monageng +5
SXP 31.0 is an X-ray source in the Small Magellanic Cloud (SMC) that was first identified as a Be X-ray Binary (BeXRB) system when it went into X-ray outbusrst in 1998. It is now k…
astro-ph.SR2020★ 7 cited
Optical and X-ray study of the peculiar high mass X-ray binary XMMU J010331.7-730144
Itumeleng M. Monageng, Malcolm J. Coe, David A. H. Buckley +6
For a long time XMMU J010331.7-730144 was proposed as a high-mass X-ray binary candidate based on its X-ray properties, however, its optical behaviour was unclear - in particular p…