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Fig. 3.

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Snapshots of the synchrotron emission maps of the jet before and after introduction of the ejecta, seen at two frequencies, ν = 1010 Hz (top) and ν = 1018 Hz (bottom). Each map represents the flux intensity in mJy units. The R and the Z axes are given in Rjet units. These maps represent the flux in the comoving frame for a viewing angle of θobs = 90° at three different comoving times (see the white boxes). The flux is evaluated at the distance of the radio galaxy 3C 111.

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