Fig. 7
Observed (crosses) and model (solid) light curves for gamma-ray (top, Fermi/LAT), X-ray continuum (middle, ASM daily mean ≥ 15 cps) and mean of SiXIV, FeXXV and FeXXVI emission lines (bottom, Chandra/HETG). The dotted lines in the two lowest panels show the contributing optical depths of the two absorbers (wind and clumpy trail), scaled with the maximum of continuum wind absorption (the same scale on the left as for the light curves).
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