  Red Geysers are quiescent galaxies with galactic scale ionised outflows,
likely due to low-luminosity Active Galactic Nuclei (AGN). We used Gemini
GMOS-IFU observations of the inner $\sim 1.0-3.0$ kpc of nine Red Geysers
selected from the MaNGA survey to study the gas ionisation and kinematics. The
emission-line ratios suggest the presence of Seyfert/LINER (Low Ionisation
Nuclear Emission Region) nuclei in all sources. Two galaxies show H$\alpha$
equivalent width (H$\alpha$ EW) larger than 3 \AA (indicative of AGN
ionisation) within an aperture 2.5 arcsec of diameter ($1.3-3.7$ kpc at the
distance of galaxies) for MaNGA data, while with the higher resolution GMOS
data, four galaxies present H$\alpha$ EW$>3$ \AA within an aperture equal to
the angular resolution ($0.3-0.9$ kpc). For two objects with GMOS-IFU data, the
H$\alpha$ EW is lower than 3 \AA but larger than 1.5 \AA, most probably due to
a faint AGN. The spatially resolved electron density maps show values between
$100-3000$ cm$^{-3}$ and are consistent with those determined in other studies.
The large (MaNGA) and the nuclear scale (GMOS-IFU) gas velocity fields are
misaligned, with a kinematic position angle difference between 12$^{\circ}$ and
60$^{\circ}$. The [NII]$\lambda$6583 emission-line profiles are asymmetrical,
with blue wings on the redshifted side of the velocity field and red wings on
the blueshifted side. Our results support previous indications that the gas in
Red Geysers is ionised by an AGN, at least in their central region, with the
presence of outflows, likely originating in a precessing accretion disc.
