Relativistic hydrodynamics simulations of supernova explosions within extragalactic jets

Open Access

Fig. A.1.

2D cuts of the 3D S1 simulation showing rest-mass density in the XY plane at z = 0, with (left panels) and without (right panels) motion of the ejecta. We selected here 3 different moments from the simulation (e.g. A.2 and 3) to show the asymmetries introduced by the orbital motion $v_{orb}^{x}$ $v^{x}_{\mathrm{orb}}$ .

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