During the 2017 giant outburst of SXP 59, the X-ray pulse profile changed from double-peaked to single-peaked as luminosity dropped, while a hot blackbody with a constant size of about 0.6 km persisted in the hard X-ray spectrum.
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NuSTAR and XMM-Newton observations of SXP 59 during its 2017 giant outburst
During the 2017 giant outburst of SXP 59, the X-ray pulse profile changed from double-peaked to single-peaked as luminosity dropped, while a hot blackbody with a constant size of about 0.6 km persisted in the hard X-ray spectrum.