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Home All issues A&A, 485 1 (2008) 177-181 Article references

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An analysis of optical periods in individual Small Magellanic Cloud Be/X-ray pulsars

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THECHANDRASURVEY OF THE SMALL MAGELLANIC CLOUD “BAR”. II. OPTICAL COUNTERPARTS OF X-RAY SOURCES

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Very long-term optical variability of high-mass X-ray binaries in the Small Magellanic Cloud

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OPTICAL SPECTROSCOPY OF 20 Be/X-RAY BINARIES IN THE SMALL MAGELLANIC CLOUD

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Highly absorbed X-ray binaries in the Small Magellanic Cloud

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XMM-Newton observations of the Small Magellanic Cloud: Be/X-ray binary pulsars active between October 2006 and June 2007

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