Fig. 12.
Simplified view of the relations among spectral components observed in NGC 3783 in X-rays: warm absorber in X-rays (WAX), broad and narrow emission lines (BEL and NEL), and emission and absorption (EM and ABS, respectively). Three different light paths are shown here. The obscurer (dashed box) is not always present along the line of sight. Dashed lines indicate that these photons are not directly observable.
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