We present the hot molecular and warm ionized gas kinematics for 33 nearby (0.001 ≲ z ≲ 0.056) X-ray selected active galaxies using the Hm and Br γ emission lines observed in the K band with the Gemini near-infrared integral field spectrograph. The observations cover the inner 0.04–2 kpc of each active galactic nucleus at spatial resolutions of 4–250 pc with a velocity resolution of σ_inst ≈ 20 . We find that 31 objects (94�per cent) present a kinematically disturbed region (KDR) seen in ionized 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 10²–10⁷ and 10⁰–10⁴ M_⊙ for the ionized and hot molecular gas, respectively. The ranges of mass-outflow rates () and kinetic power () of the outflows are 10⁻³–10¹ M_⊙ yr⁻¹ and ∼10³⁷–10⁴³ erg s⁻¹ for the ionized gas outflows, and 10⁻⁵–10⁻² M_⊙ yr⁻¹ and 10³⁵–10³⁹ erg s⁻¹ for the hot molecular gas outflows. The median coupling efficiency in our sample is and the estimated momentum fluxes of the outflows suggest they are produced by radiation-pressure in low-density environment, with possible contribution from shocks.