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We analyzed near-infrared data of the nearby galaxy IC5063 taken with theVery Large Telescope SINFONI instrument. IC5063 is an elliptical galaxy thathas a radio jet nearly aligned with the major axis of a gas disk in its center.The data reveal multiple signatures of molecular and atomic gas that has beenkinematically distorted by the passage of the jet plasma or cocoon within anarea of ~1 kpc^2. Concrete evidence that the interaction of the jet with thegas causes the gas to accelerate comes from the detection of outflows in fourdifferent regions along the jet trail: near the two radio lobes, between theradio emission tip and the optical narrow-line-region cone, and at a regionwith diffuse 17.8 GHz emission midway between the nucleus and the north radiolobe. The outflow in the latter region is biconical, centered 240 pc away fromthe nucleus, and oriented perpendicularly to the jet trail. The diffuseemission that is observed as a result of the gas entrainment or scatteringunfolds around the trail and away from the nucleus with increasing velocity. Itoverall extends for >700 pc parallel and perpendicular to the trail. Near theoutflow starting points, the gas has a velocity excess of 600 km/s to 1200 km/swith respect to ordered motions, as seen in [FeII], Pa alpha, or H2 lines. HighH2 (1-0) S(3)/S(1) flux ratios indicate non-thermal excitation of gas in thediffuse outflow.

A radio jet drives a molecular and atomic gas outflow in multiple regions within one square kiloparsec of the nucleus of the nearby galaxy IC5063