Traces of wobbling accretion disk in X-ray pulsar Her X-1 from observations of the ART-XC telescope of the SRG observatory

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Fig. 11.

Top: 4–12 keV light curve of the exponential flux growth. Middle panel: Corresponding 12–25 keV light curve. Bottom panel: softness of the X-ray light curve during the emission growth after the main turn-on. Red dots mark the X-ray dip as in Figs. 9–10.

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