  NGC 7469 is a well known Luminous IR Galaxy, with a circumnuclear star
formation ring ($\sim 830$ pc radius) surrounding a Seyfert 1 AGN. Nuclear
unresolved winds were previously detected in X-rays and UV, as well as an
extended biconical outflow in IR coronal lines. We search for extended outflows
by measuring the kinematics of the $\mathrm{H\beta}$ and [O III] $\lambda 5007$
optical emission lines, in data of the VLT/MUSE integral field spectrograph. We
find evidence of two outflow kinematic regimes: one slower regime extending
across most of the star formation ring -- possibly driven by the massive star
formation -- and a faster regime (with a maximum velocity of $-715 \ \mathrm{km
\ s^{-1}}$), only observed in [O III], in the western region between the AGN
and the massive star forming regions of the ring, likely AGN-driven. This work
shows a case where combined AGN/star-formation feedback can be effectively
spatially-resolved, opening up a promising path toward a deeper understanding
of feedback processes in the central kiloparsec of AGN.
