Figure 5 from Blazar Variability from Turbulence in Jets Launched by Magnetically Arrested Accretion Flows

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Blazar Variability from Turbulence in Jets Launched by Magnetically Arrested Accretion Flows

Authors: Michael O' Riordan, Asaf Pe'er, and Jonathan C. McKinney

2017 The Astrophysical Journal 843 81.

Provider: AAS Journals

Caption: Figure 5.

Same as Figure 3 but showing the simulated PDS for the optical band. In this case, the light curves are dominated by synchrotron emission. The observational data again corresponds to energies ﹩\gt 100\,\mathrm{MeV}﹩. It is clear that optical PDS shows a similar power-law behavior to that in the γ-rays.

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