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Properties of X-ray Binaries in the Magellanic Clouds from RXTE and Chandra Observations
R. H. D. Corbet, M. J. Coe, K. E. McGowan +4
The X-ray binary population of the SMC is very different from that of the Milky Way consisting, with one exception, entirely of transient pulsating Be/neutron star binaries. We hav…
High mass X-ray binary SXP18.3 undergoes the longest Type II outburst ever seen in the Small Magellanic Cloud
M. P. E. Schurch, M. J. Coe, J. L. Galache +6
On 30th August 2006 SXP18.3 a high mass X-ray binary (HMXB) in the Small Magellanic Cloud (SMC) with an 18.3s pulse period was observed by Rossi X-ray Timing Explorer (RXTE). The s…
Optical properties of High-Mass X-ray Binaries (HMXB) in the Small Magellanic Cloud
M. J. Coe, R. H. D. Corbet, K. E. McGowan +6
The SMC represents an exciting opportunity to observe the direct results of tidal interactions on star birth. One of the best indicators of recent star birth activity is the presen…
XMM-Newton observations of the Small Magellanic Cloud: XMMU J004814.1-731003, a 25.55 s Be/X-ray binary pulsar
F. Haberl, P. Eger, W. Pietsch +2
To investigate candidates for Be/X-ray binaries in the Small Magellanic Cloud (SMC), we observed a region around the emission nebula N19 with XMM-Newton in October 2006. We analyse…
A Long Look at the Be/X-Ray Binaries of the Small Magellanic Cloud
J. L. Galache, R. H. D. Corbet, M. J. Coe +5
We have monitored 41 Be/X-ray binary systems in the Small Magellanic Cloud over ~9 years using PCA-RXTE data from a weekly survey program. The resulting light curves were analysed…