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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 4.

Three components of vorticity (﹩{\omega }_{x},\;﹩ ﹩{\omega }_{y},\;﹩ ﹩{\omega }_{z}﹩ from left to right) for a snapshot of the domain in the fiducial case at ﹩t=140h/{c}_{{\rm{iso,0}}}.﹩ The color table is set so that green is ﹩{\omega }_{x,y,z}=0,\;﹩ and red/blue saturate at ﹩{\omega }_{x,y,z}=\pm 0.2.﹩

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