Image Details

Choose export citation format:

How Does Radio AGN Feedback Feed Back?

  • Authors: David S. De Young

DE YOUNG 2010 The Astrophysical Journal 710 743.

  • Provider: AAS Journals

Caption: Figure 3.

Turbulent kinetic energy spectra at a scaled time of t = 60 for a wavenumber space extending to k = 1024. Shown are the spectra for delta function and Gaussian energy injection profiles, with the form of the Gaussian injection spectrum also shown. No appreciable differences exist in the overall energy spectrum for the two different injection profiles.

Other Images in This Article
Copyright and Terms & Conditions