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We use Gemini Multi-Object Spectrograph (GMOS) Integral Field Unit (IFU)observations of the inner 285$\times$400 pc$^2$ region of the Seyfert 2 galaxyNGC 5643 to map the [SIII]$\lambda9069$ emission-line flux distribution andkinematics, as well as the stellar kinematics, derived by fitting theCaII$\lambda\lambda\lambda$8498,8542,8662 triplet, at a spatial resolution of45 pc. The stellar velocity field shows regular rotation, with a projectedvelocity of 100 km/s and kinematic major axis along Position Angle$PA=-36^\circ$. A ring of low stellar velocity dispersion values ($\sim$70km/s), attributed to young/intermediate age stellar populations, is seensurrounding the nucleus with radius of 50 pc. We found that the [SIII] fluxdistribution shows an elongated structure along the east-west direction and itskinematics is dominated by outflows within a bi-cone at an ionized gas outflowrate of 0.3 M$_\odot$ yr$^{-1}$. In addition, velocity slices across the[SIII]$\lambda9069$ emission-line reveal a kinematic component attributed torotation of gas in the plane of the galaxy.

Outflows in the Seyfert 2 galaxy NGC5643 traced by the [SIII] emission