Fig. 11.
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High/soft spectral state of Cygnus X-1 as observed by RXTE, ASCA, and NuSTAR (Ling et al. 1997; Dotani et al. 1997; Walton et al. 2016). The observational data are fitted by a blackbody spectrum emitted by the inner disk region and an IC-scattered component of the disk emission off a combination of thermal and nonthermal corona electrons.
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