The orbital solution and spectral classification of the high-mass X-ray binary IGR J01054−7253 in the Small Magellanic Cloud

We present X-ray and optical data on the Be/X-ray binary (BeXRB) pulsar IGR J 01054−7253= SXP11.5 in the Small Magellanic Cloud (SMC). Rossi X-ray Timing Explorer (RXTE) observations of this source in a large X-ray outburst reveal an 11.483 ± 0.002 s pulse period and show both the accretion-driven s...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2011-01, Vol.410 (3), p.1813-1824
Hauptverfasser:	Townsend, L. J., Coe, M. J., Corbet, R. H. D., McBride, V. A., Hill, A. B., Bird, A. J., Schurch, M. P. E., Haberl, F., Sturm, R., Pathak, D., van Soelen, B., Bartlett, E. S., Drave, S. P., Udalski, A.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Binary system Earth, ocean, space ephemerides Exact sciences and technology line line, Be Luminosity Magellanic Clouds Neutrons Pulsars Spectrum analysis stars: emission X-ray astronomy X-rays: binaries
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