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Insights on the Origin of Odd Radio Circles from Cosmological Simulations

  • Authors: Klaus Dolag, Ludwig M. Böss, Bärbel S. Koribalski, Ulrich P. Steinwandel, Milena Valentini

Klaus Dolag et al 2023 The Astrophysical Journal 945 .

  • Provider: AAS Journals

Caption: Figure 9.

Total synchrotron brightness of the simulated ORC within a radius of r < 500h −1 cMpc for our chosen CR acceleration efficiencies models. We use a constant magnetic field strength of B = 5 μG for all synchrotron emitting particles. Note that the observed synchrotron power at 944 MHz for ORC 5 is significantly larger, e.g., ≈5.5 × 1023 W Hz−1 (Koribalski et al. 2021).

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