Journal Article

<i>INTEGRAL</i> deep observations of the Small Magellanic Cloud

M. J. Coe, A. J. Bird, D. A. H. Buckley, R. H. D. Corbet, A. J. Dean, M. Finger, J. L. Galache, F. Haberl, V. A. McBride, I. Negueruela, M. Schurch, L. J. Townsend, A. Udalski, J. Wilms and A. Zezas

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 406, issue 4, pages 2533-2539
Published in print August 2010 | ISSN: 0035-8711
Published online August 2010 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2010.16844.x
INTEGRAL deep observations of the Small Magellanic Cloud

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Deep observations of the Small Magellanic Cloud (SMC) and region were carried out in the hard X-ray band by the INTEGRAL observatory in 2008–2009. The field of view of the instrument permitted simultaneous coverage of the entire SMC and the eastern end of the Magellanic Bridge. In total, INTEGRAL detected seven sources in the SMC and five in the Magellanic Bridge; the majority of the sources were previously unknown systems. Several of the new sources were detected undergoing bright X-ray outbursts and all the sources exhibited transient behaviour except the supergiant system SMC X-1. They are all thought to be high-mass X-ray binary systems in which the compact object is a neutron star.

Keywords: stars: neutron; X-rays: binaries

Journal Article.  4188 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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