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A long look at the Be/X-ray binaries of the small magellanic cloud

A long look at the Be/X-ray binaries of the small magellanic cloud
A long look at the Be/X-ray binaries of the small magellanic cloud
We have monitored 41 Be/X-ray binary systems in the Small Magellanic Cloud over ~9 yr using PCA RXTE data from a weekly survey program. The resulting light curves were analyzed in search of orbital modulations with the result that 10 known orbital ephemerides were confirmed and refined, while 10 new ones where determined. A large number of X-ray orbital profiles are presented for the first time, showing similar characteristics over a wide range of orbital periods. Lastly, three pulsars, SXP 46.4, SXP 89.0, and SXP 165, were found to be misidentifications of SXP 46.6, SXP 91.1, and SXP 169, respectively.
0067-0049
189-215
Galache, J.L.
f4b15a28-e3a7-49bb-9000-4e75df9d93ad
Corbet, R.H.D.
7d365a78-a577-4f56-8d3a-503b7fccb42b
Coe, M.J.
04dfb23b-1456-46a3-9242-5cee983471d5
Laycock, S.
3021ea8f-9d14-4cda-93cd-6776c37ed386
Schurch, M.P.E.
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Markwardt, C.
42b907ed-dbe4-4e4f-b80b-554ec69bcb0e
Marshall, F.E.
78772a43-cdce-42b8-96c9-5f2d355ac482
Lochner, J.
a393ad57-d085-46c9-89f5-720a8cd1cc13
Galache, J.L.
f4b15a28-e3a7-49bb-9000-4e75df9d93ad
Corbet, R.H.D.
7d365a78-a577-4f56-8d3a-503b7fccb42b
Coe, M.J.
04dfb23b-1456-46a3-9242-5cee983471d5
Laycock, S.
3021ea8f-9d14-4cda-93cd-6776c37ed386
Schurch, M.P.E.
1a6b3c0a-67d7-44e9-9d0c-94041f939d6b
Markwardt, C.
42b907ed-dbe4-4e4f-b80b-554ec69bcb0e
Marshall, F.E.
78772a43-cdce-42b8-96c9-5f2d355ac482
Lochner, J.
a393ad57-d085-46c9-89f5-720a8cd1cc13

Galache, J.L., Corbet, R.H.D., Coe, M.J., Laycock, S., Schurch, M.P.E., Markwardt, C., Marshall, F.E. and Lochner, J. (2008) A long look at the Be/X-ray binaries of the small magellanic cloud. The Astrophysical Journal Supplement Series, 177 (1), 189-215. (doi:10.1086/587743).

Record type: Article

Abstract

We have monitored 41 Be/X-ray binary systems in the Small Magellanic Cloud over ~9 yr using PCA RXTE data from a weekly survey program. The resulting light curves were analyzed in search of orbital modulations with the result that 10 known orbital ephemerides were confirmed and refined, while 10 new ones where determined. A large number of X-ray orbital profiles are presented for the first time, showing similar characteristics over a wide range of orbital periods. Lastly, three pulsars, SXP 46.4, SXP 89.0, and SXP 165, were found to be misidentifications of SXP 46.6, SXP 91.1, and SXP 169, respectively.

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Published date: July 2008
Organisations: Physics & Astronomy

Identifiers

Local EPrints ID: 143573
URI: http://eprints.soton.ac.uk/id/eprint/143573
ISSN: 0067-0049
PURE UUID: 9321357a-9419-473f-8c66-c4f3a115ee3d
ORCID for M.J. Coe: ORCID iD orcid.org/0000-0002-0763-8547

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Date deposited: 12 Apr 2010 13:39
Last modified: 14 Mar 2024 02:32

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Contributors

Author: J.L. Galache
Author: R.H.D. Corbet
Author: M.J. Coe ORCID iD
Author: S. Laycock
Author: M.P.E. Schurch
Author: C. Markwardt
Author: F.E. Marshall
Author: J. Lochner

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