  We present spatially resolved gas kinematics, ionization, and energetics of
11 type 1 and 5 type 2 active galactic nuclei (AGNs) with strong ionized gas
outflows at z $<0.3$ using Gemini Multi-Object Spectrograph Integral Field Unit
(GMOS-IFU) data. We find a strongly blueshifted region in [OIII] velocity maps,
representing an approaching cone in biconical outflows, and blueshifted and
redshifted regions in H$\alpha$ velocity maps, which show gravitationally
rotating kinematics. AGN photoionization is dominant in the central region of
most targets, and some of them also show ring-like structures of LINER or
composite that surround the AGN-dominated center. Following our previous
studies, we kinematically determine outflow sizes by the ratio between [OIII]
and stellar velocity dispersion. Outflow sizes of type 1 AGNs follow the same
kinematic outflow size-[OIII] luminosity relation obtained from the type 2 IFU
sample in Kang & Woo and Luo (updated slope $0.29\pm0.04$), while they are
limited to the central kpc scales, indicating the lack of global impact of
outflows on the interstellar medium. Small mass outflow rates and large star
formation rates of the combined sample support that there is no evidence of
rapid star formation quenching by outflows, which is consistent with the
delayed AGN feedback.
