  We present the hot molecular and warm ionised gas kinematics for 33 nearby
($0.001\lesssim z\lesssim0.056$) X-ray selected active galaxies using the H$_2
2.1218 \mu$m and Br$\gamma$ emission lines observed in the K-band with the
Gemini Near-Infrared Field Spectrograph (NIFS). The observations cover the
inner 0.04$-$2 kpc of each AGN at spatial resolutions of 4$-$250 pc with a
velocity resolution of $\sigma_{\rm inst}\approx$20 ${\rm km s^{-1}}$. We find
that 31 objects (94 per cent) present a kinematically disturbed region (KDR)
seen in ionised gas, while such regions are observed in hot molecular gas for
25 galaxies (76 per cent). We interpret the KDR as being due to outflows with
masses of 10$^2-$10$^7$ M$_\odot$ and 10$^0-$10$^4$ M$_\odot$ for the ionised
and hot molecular gas, respectively. The ranges of mass-outflow rates
($\dot{M}_{\rm out}$) and kinetic power ($\dot{E}_{\rm K}$) of the outflows are
10$^{-3}-$10$^{1}$ M$_\odot$yr$^{-1}$ and $\sim$10$^{37}$$-$10$^{43}$ erg
s$^{-1}$ for the ionised gas outflows, and 10$^{-5}$$-$10$^{-2}$ M$_\odot$
yr$^{-1}$ and 10$^{35}$$-$10$^{39}$ erg s$^{-1}$ for the hot molecular gas
outflows. The median coupling efficiency in our sample is $\dot{E}_{K}/L_{\rm
bol}\approx1.8\times10^{-3}$ and the estimated momentum fluxes of the outflows
suggest they are produced by radiation-pressure in low-density environment,
with possible contribution from shocks.
