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INEFFICIENT DRIVING OF BULK TURBULENCE BY ACTIVE GALACTIC NUCLEI IN A HYDRODYNAMIC MODEL OF THE INTRACLUSTER MEDIUM

  • Authors: Christopher S. Reynolds, Steven A. Balbus, and Alexander A. Schekochihin

2015 The Astrophysical Journal 815 41.

  • Provider: AAS Journals

Caption: Figure 1.

Three-dimensional renderings of the lower half (﹩z\lt 4h﹩) of the domain in the fiducial case (﹩{z}_{0}=10h﹩) at two times, ﹩t=84h/{c}_{{\rm{iso,0}}}﹩ (left) and ﹩t=180h/{c}_{{\rm{iso,0}}}﹩ (right). We show the magnitude of the full velocity as orange shading on representative slices. Shown in blue is a volume rendering of the injected tracer ﹩{\mu }_{1},\;﹩ which flags the region polluted by the debris of the AGN-blown bubbles.

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