Gas inflows towards the nucleus of NGC1358
  We use optical spectra from the inner 1.8 $\times$ 2.5kpc$^2$ of the Seyfert
2 galaxy NGC1358, obtained with the GMOS integral field spectrograph on the
Gemini South telescope at a spatial resolution of $\approx$ 165pc, to assess
the feeding and feedback processes in this nearby active galaxy. Five gaseous
kinematical components are observed in the emission line profiles. One of the
components is present in the entire field-of-view and we interpret it as due to
gas rotating in the disk of the galaxy. Three of the remaining components we
interpret as associated to active galactic nucleus (AGN) feedback: a compact
unresolved outflow in the inner 1 arcsec and two gas clouds observed at
opposite sides of the nucleus, which we propose have been ejected in a previous
AGN burst. The disk component velocity field is strongly disturbed by a large
scale bar. The subtraction of a velocity model combining both rotation and bar
flows reveals three kinematic nuclear spiral arms: two in inflow and one in
outflow. We estimate the mass inflow rate in the inner 180pc obtaining
$\dot{M}_{in}$ $\approx$ 1.5 $\times 10^{-2}$M$_{\odot}$yr$^{-1}$, about 160
times larger than the accretion rate necessary to power this AGN.
