Image Details
Caption: Figure 2.
Thermal Stability (S-Curve) for the photoionization models; same as above with the red triangles showing two states of the highest ionization warm absorber in NGC 4151 (XHIGH; Couto et al. 2016). Note that the three types of absorbers occupy different regions of the S-curve, with the UFOs primarily on the flat, Compton-dominated section.
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