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Cited article:
P. Eger , F. Haberl
A&A, 485 3 (2008) 807-811
Published online: 2008-05-15
This article has been cited by the following article(s):
5 articles
eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds
F. Haberl, C. Maitra, S. Carpano, et al. Astronomy & Astrophysics 661 A25 (2022) https://doi.org/10.1051/0004-6361/202141878
High-mass X-ray binaries in the Small Magellanic Cloud
F. Haberl and R. Sturm Astronomy & Astrophysics 586 A81 (2016) https://doi.org/10.1051/0004-6361/201527326
An analysis of optical periods in individual Small Magellanic Cloud Be/X-ray pulsars
P. C. Schmidtke, A. P. Cowley and A. Udalski Monthly Notices of the Royal Astronomical Society 431 (1) 252 (2013) https://doi.org/10.1093/mnras/stt159
EXPLORING THE SMALL MAGELLANIC CLOUD TO THE FAINTEST X-RAY FLUXES: SOURCE CATALOG, TIMING, AND SPECTRAL ANALYSIS
Silas Laycock, Andreas Zezas, Jaesub Hong, Jeremy J. Drake and Valsamo Antoniou The Astrophysical Journal 716 (2) 1217 (2010) https://doi.org/10.1088/0004-637X/716/2/1217
XMM-Newton observations of the Small Magellanic Cloud:
Long term evolution of frequently observed Be/X-ray binaries
P. Eger and F. Haberl Astronomy & Astrophysics 491 (3) 841 (2008) https://doi.org/10.1051/0004-6361:200810809