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*AIMS: To study the interaction between young AGN and their host galaxiesbased on their ionized gas and radio emission, and to analyze possibleimplications for the radio galaxy evolution.  *METHODS: The [OIII] 5007 line and 5-GHz radio properties are compared andstudied on a large, representative sample of GPS and CSS (i.e., young) quasarsand radio galaxies as well as large-scale sources using [OIII] 5007 line and5-GHz radio data from literature and our observations.  *RESULTS: Several correlations between the [OIII] 5007 line and 5-GHz radioemission have been found. The main result is that the [OIII] 5007 emission isstrongly related to the GPS/CSS source size indicating that the [OIII] 5007emission is clearly enhanced by the jet expansion through the host galaxy ISM.Shocks are the most likely enhancing mechanism, although jet-induced starformation could also be, partly, responsible for the [OIII] 5007 emission. Thedata also suggests a possible deceleration of the jet as it grows. In thiscase, however, the correlation is weak.

Tracing jet--ISM interaction in young AGN: correlations between [OIII] 5007 and 5-GHz emission