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Physical Conditions in Ultra-fast Outflows in AGN

  • Authors: S. B. Kraemer, F. Tombesi, and M. C. Bottorff

2018 The Astrophysical Journal 852 35.

  • Provider: AAS Journals

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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