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

Open Access

Fig. 5.

Top: ART-XC Her X-1 a hard spectrum in the low state (see also Fig. 4). Dashed gray lines indicate models HIGHECUT(POWERLAW), GAUSSIAN, AND BLACKBODY. Dashed black line is the total model. Bottom: difference between the observation points and the total model.

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