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High-resolution (0.5 arcsec) CO(2-1) observations performed with the AtacamaLarge Millimetre/submillimetre Array have been used to trace the kinematics ofthe molecular gas in the Seyfert 2 galaxy{IC~5063}. Although one of the mostradio-loud Seyfert galaxy, IC~5063 is a relatively weak radio source (P_1.4GHz= 3 x 10^23 W Hz^-1). The data reveal that the kinematics of the gas is verycomplex. A fast outflow of molecular gas extends along the entire radio jet (~1 kpc), with the highest outflow velocities about 0.5 kpc from the nucleus, atthe location of the brighter hot-spot in the W lobe. All the observedcharacteristics can be described by a scenario of a radio plasma jet expandinginto a clumpy medium, interacting directly with the clouds and inflating acocoon that drives a lateral outflow into the interstellar medium. Thissuggests that most of the observed cold molecular outflow is due to fastcooling of the gas after the passage of a shock and that it is the end productof the cooling process.

Radio Jets Clearing theWay Through a Galaxy: Watching Feedback in Action in the Seyfert galaxy IC 5063