Simulating radio emission from flickering AGN jets: travelling shocks and hotspot brightening
Published in Monthly Notices of the Royal Astronomical Society, 2026
We investigate the impact of flickering variability in jet power on the luminosity and morphology of radio galaxies. We use a Lagrangian particle method together with relativistic hydrodynamics simulations using the PLUTO code to track the evolution of electron spectra through particle acceleration at shocks and cooling processes.
Recommended citation: Elley, Emma L., Matthews, James H., Mukherjee, Dipanjan & Vaidya, Bhargav (2009). "Simulating radio emission from flickering AGN jets: travelling shocks and hotspot brightening." Monthly Notices of the Royal Astronomical Society. 546(2).
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