The XMM-Newton survey of the small magellanic cloud: XMMUJ005011.2-730026 = SXP214, a Be/X-ray binary pulsar

Article


Coe, M. J., Haberl, F., Sturm, R., Pietsch, W., Townsend, L. J., Bartlett, E. S., Filipovic, M., Udalski, A., Corbet, R. H. D., Tiengo, A., Ehle, M., Payne, J. L. and Burton, D.. 2011. "The XMM-Newton survey of the small magellanic cloud: XMMUJ005011.2-730026 = SXP214, a Be/X-ray binary pulsar." Monthly Notices of the Royal Astronomical Society. 414 (4), pp. 3281-3287. https://doi.org/10.1111/j.1365-2966.2011.18626.x
Article Title

The XMM-Newton survey of the small magellanic cloud: XMMUJ005011.2-730026 = SXP214, a Be/X-ray binary pulsar

ERA Journal ID1074
Article CategoryArticle
AuthorsCoe, M. J. (Author), Haberl, F. (Author), Sturm, R. (Author), Pietsch, W. (Author), Townsend, L. J. (Author), Bartlett, E. S. (Author), Filipovic, M. (Author), Udalski, A. (Author), Corbet, R. H. D. (Author), Tiengo, A. (Author), Ehle, M. (Author), Payne, J. L. (Author) and Burton, D. (Author)
Journal TitleMonthly Notices of the Royal Astronomical Society
Journal Citation414 (4), pp. 3281-3287
Number of Pages7
Year2011
PublisherOxford University Press
Place of PublicationUnited Kingdom
ISSN0035-8711
1365-2966
Digital Object Identifier (DOI)https://doi.org/10.1111/j.1365-2966.2011.18626.x
Web Address (URL)https://academic.oup.com/mnras/article/414/4/3281/996207
Abstract

In the course of the XMM-Newton survey of the Small Magellanic Cloud (SMC), a region to the east of the emission nebula N19 was observed in November 2009. To search for new candidates for high mass X-ray binaries the EPIC PN and MOS data of the detected point sources were investigated and their spectral and temporal characteristics identified. A new transient (XMMUJ005011.2-730026= SXP214) with a pulse period of 214.05 s was discovered; the source had a hard X-ray spectrum with power-law index of ~0.65. The accurate X-ray source location permits the identification of the X-ray source with a ~15th magnitude Be star, thereby confirming this system as a new Be/X-ray binary.

Keywordsstars; neutron; X-rays; binaries
ANZSRC Field of Research 2020401303. Navigation and position fixing
490302. Numerical analysis
510104. Galactic astronomy
Public Notes

This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2011 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.

Institution of OriginUniversity of Southern Queensland
Byline AffiliationsUniversity of Southampton, United Kingdom
Max Planck Society, Germany
University of Western Sydney
University of Warsaw, Poland
NASA Goddard Space Flight Centre, United States
Institute of Space Astrophysics and Cosmic Physics, Italy
European Space Agency, France
Faculty of Sciences
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