We present optical integral field spectroscopy of the circum-nuclear gas of the Seyfert 2 galaxy NGC 1386 .
The data cover the central 7 ^ { \prime \prime } \times 9 ^ { \prime \prime } ( 530 \times 680 pc ) at a spatial resolution of 0 \farcs 9 ( 68 pc ) , and the spectral range 5700-7000 Ã Â at a resolution of 66 km s ^ { -1 } .
The line emission is dominated by a bright central component , with two lobes extending \approx 3 ^ { \prime \prime } north and south of the nucleus .
We identify three main kinematic components .
The first has low velocity dispersion ( \bar { \sigma } \approx 90 km s ^ { -1 } ) , extends over the whole field-of-view , and has a velocity field consistent with gas rotating in the galaxy disk .
We interpret the lobes as resulting from photoionization of disk gas in regions where the AGN radiation cones intercept the disk .
The second has higher velocity dispersion ( \bar { \sigma } \approx 200 km s ^ { -1 } ) and is observed in the inner 150 pc around the continuum peak .
This component is double peaked , with redshifted and blueshifted components separated by \approx 500 km s ^ { -1 } .
Together with previous HST imaging , these features suggest the presence of a bipolar outflow for which we estimate a mass outflow rate of \mathrm { \dot { M } } \gtrsim 0.1 M _ { \odot } yr ^ { -1 } .
The third component is revealed by velocity residuals associated with enhanced velocity dispersion and suggests that outflow and/or rotation is occurring approximately in the equatorial plane of the torus .
A second system of velocity residuals may indicate the presence of streaming motions along dusty spirals in the disk .