Fig. 6
X-ray lightcurves of WR 46 (background subtracted, binned in 1000 s intervals) in two different energy bands. Upper panel: WR 46 in the 0.2−0.5 keV band; Middle panel: background near the star in the same band; Lower panel: WR 46 in the 0.5−2.0 keV band. The lightcurve corresponds to the combination of the three EPIC instruments (uncleaned event lists). The abscissae give the elapsed time expressed in s; the origin of the time is arbitrary.
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