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The Impact of a Clumpy Ambient Medium on the Dynamics and Synchrotron Emission of AGN Jets
Relativistic jets from AGN are expected to propagate through an inhomogeneous ISM, but the role of small-scale gas inhomogeneities in shaping their early evolution remains uncertain. We investigate this problem using 3D special-relativistic magnetohydrodynamic simulations with PLUTO, following a jet
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