  Energetic ionized gas outflows driven by active galactic nuclei (AGN) have
been studied as a key phenomenon related to AGN feedback. To probe the
kinematics of the gas in the narrow line region, [O III] ${\lambda}$5007 has
been utilized in a number of studies, showing non-virial kinematic properties
due to AGN outflows. In this paper, we statistically investigate whether the
H-alpha emission line is influenced by AGN driven outflows, by measuring the
kinematic properties based on the H-alpha line profile, and by comparing them
with those of [O III]. Using the spatially integrated spectra of ~37,000 Type 2
AGNs at z < 0.3 selected from the SDSS DR7, we find a non-linear correlation
between H-alpha velocity dispersion and stellar velocity dispersion, which
reveals the presence of the non-gravitational component, especially for AGNs
with a wing component in H-alpha. The large H-alpha velocity dispersion and
velocity shift of luminous AGNs are clear evidence of AGN outflow impacts on
hydrogen gas, while relatively smaller kinematic properties compared to those
of [O III] imply that the observed outflow effect on the H-alpha line is weaker
than the case of [O III].
