Fig. 2.
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Pulse profiles of Cen X-3 in 3–78 keV from the summations of the FPMA and FPMB counts. These profiles are aligned by defining the minimum as phase zero. The first panel is from the first time interval. The second panel comes from intervals 2 to 13 in the first orbit with a moderate luminosity. The third panel comes from intervals 14 to 23 in the second orbit with high luminosity.
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