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Integral deep observations of the small magellanic cloud

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.
045ee141-4720-46fd-a412-5aa848a91b32
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)

Record type: Article

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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More information

Submitted date: 13 April 2010
Additional Information: Imported from arXiv

Identifiers

Local EPrints ID: 144745
URI: http://eprints.soton.ac.uk/id/eprint/144745
PURE UUID: 36f14769-747f-40d2-8d57-7be406176024
ORCID for Malcolm J. Coe: ORCID iD orcid.org/0000-0002-0763-8547
ORCID for Anthony J. Bird: ORCID iD orcid.org/0000-0002-6888-8937

Catalogue record

Date deposited: 24 May 2010 12:09
Last modified: 11 Dec 2021 02:55

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Contributors

Author: Malcolm J. Coe ORCID iD
Author: Anthony J. Bird ORCID iD
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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