Integral deep observations of the small magellanic cloud
Integral deep observations of the small magellanic cloud
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 (HMXB) systems in which the compact object is a neutron star.
Coe, Malcolm J.
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Bird, Anthony J.
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Buckley, D.A.H.
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Corbet, R.H.D.
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Dean, Anthony J.
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Finger, M.
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Galache, José L.
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Haberl, Frank
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McBride, Vanessa
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Negueruela, I.
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Schurch, Matthew
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Townsend, Lee J.
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Udalski, A.
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Wilms, J.
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Zezas, A.
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Coe, Malcolm J.
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Bird, Anthony J.
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Buckley, D.A.H.
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Corbet, R.H.D.
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Dean, Anthony J.
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Finger, M.
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Galache, José L.
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Haberl, Frank
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McBride, Vanessa
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Negueruela, I.
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Schurch, Matthew
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Townsend, Lee J.
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Udalski, A.
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Wilms, J.
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Zezas, A.
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Coe, Malcolm J., Bird, Anthony J., Buckley, D.A.H., Corbet, R.H.D., Dean, Anthony J., Finger, M., Galache, José L., Haberl, Frank, McBride, Vanessa, Negueruela, I., Schurch, Matthew, Townsend, Lee J., Udalski, A., Wilms, J. and Zezas, A.
(2010)
Integral deep observations of the small magellanic cloud.
Pre-print, (arXiv:1004.221).
(Submitted)
Abstract
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 (HMXB) systems in which the compact object is a neutron star.
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Submitted date: 13 April 2010
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Imported from arXiv
Identifiers
Local EPrints ID: 144745
URI: http://eprints.soton.ac.uk/id/eprint/144745
PURE UUID: 36f14769-747f-40d2-8d57-7be406176024
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Date deposited: 24 May 2010 12:09
Last modified: 11 Dec 2021 02:55
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Contributors
Author:
D.A.H. Buckley
Author:
R.H.D. Corbet
Author:
Anthony J. Dean
Author:
M. Finger
Author:
José L. Galache
Author:
Frank Haberl
Author:
Vanessa McBride
Author:
I. Negueruela
Author:
Matthew Schurch
Author:
Lee J. Townsend
Author:
A. Udalski
Author:
J. Wilms
Author:
A. Zezas
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