NASA NTRS · 20030109435
XTE JO111.2-7317: An X-Ray Binary in the SMC
Abstract
The observed characteristics of the nebulosity surrounding the SMC High Mas X-ray Binary XTE J0111.2-7316 are examined in the context of three possible nebular types: SNR, bowshock and HII region. Observational evidence is presented which appears to support the interpretation that the nebulosity surrounding XTE JO111.2-7316 is an HII region. The source therefore appears to be a normal SMC BeXRB embedded in a locally enhanced ISM which it has photoionised to create an HII region.
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Coe, M. J., Haigh, N. J., Wilson, C. A., Negueruela, I.. 2003-01-01. XTE JO111.2-7317: An X-Ray Binary in the SMC. https://ntrs.nasa.gov/citations/20030109435
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