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XTE JO111.2-7317: An X-Ray Binary in the SMCThe 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.
Document ID
20030109435
Acquisition Source
Marshall Space Flight Center
Document Type
Abstract
Authors
Coe, M. J. (Southampton Univ. United Kingdom)
Haigh, N. J. (Southampton Univ. United Kingdom)
Wilson, C. A. (NASA Marshall Space Flight Center Huntsville, AL, United States)
Negueruela, I.
Date Acquired
August 21, 2013
Publication Date
January 1, 2003
Subject Category
Astronomy
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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