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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 3.

Ratio of ﹩{v}_{{\rm{z}}}﹩ to the Kelperian velocity at the footprint of the flow, plotted against χ, for launch angles ﹩{\theta }_{{\rm{o}}}=20^\circ ﹩ (solid), ﹩30^\circ ﹩ (dotted), and ﹩40^\circ ﹩ (dashed). The Alfvén critical points (X) and position of the UFO (U) are indicated for all three. Note that for ﹩{\theta }_{{\rm{o}}}=40^\circ ﹩, the UFO is at a sub-Alfvénic point.

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