  The emission lines in the active galaxy IRAS 0421+0400 show a dramatic (~ 900
km/s) increase in the velocity spread at the position of radio hotspots which
are located at the beginning of extended radio lobes. We study a model which
explains this phenomenon as the result of a jet emerging through the boundary
between the interstellar and intergalactic media. A similar scenario has
previously been suggested as an explanation for wide angle tail radio sources
(WATs). Based on our model, we simulate the longslit spectra of these regions
and compare the results with the observations and find that it can explain most
of the details in the observed longslit spectra.
