Outflows in the Seyfert 2 galaxy NGC5643 traced by the [SIII] emission
  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 galaxy
NGC 5643 to map the [SIII]$\lambda9069$ emission-line flux distribution and
kinematics, as well as the stellar kinematics, derived by fitting the
CaII$\lambda\lambda\lambda$8498,8542,8662 triplet, at a spatial resolution of
45 pc. The stellar velocity field shows regular rotation, with a projected
velocity of 100 km/s and kinematic major axis along Position Angle
$PA=-36^\circ$. A ring of low stellar velocity dispersion values ($\sim$70
km/s), attributed to young/intermediate age stellar populations, is seen
surrounding the nucleus with radius of 50 pc. We found that the [SIII] flux
distribution shows an elongated structure along the east-west direction and its
kinematics is dominated by outflows within a bi-cone at an ionized gas outflow
rate of 0.3 M$_\odot$ yr$^{-1}$. In addition, velocity slices across the
[SIII]$\lambda9069$ emission-line reveal a kinematic component attributed to
rotation of gas in the plane of the galaxy.
