Fig. 5
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Light curves for a smooth stellar wind for the adiabatic (green dashed) and radiative (blue solid) regimes including regions of the CD up to 1.5d from the star for synchrotron emission in the 1–100 keV band (top) and IC emission in the 0.1–10 GeV (middle) and >100 GeV (bottom) energy bands. The vertical dashed lines labeled SUP and INF mark the superior and inferior conjunction, respectively. We show two orbital cycles for clarity.
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