Abstract
We present preliminary results related to the ionized gas kinematics of the Local Group dwarf irregular galaxy IC 10. Our main goal is to study the interaction between the gas and stars in this object. Scanning Fabry-Perot interferometry was performed in the Hα, [SII], [NII] and [OIII] lines to a moderate spectral sampling ∼ 19 km s^{-1} and spatial ∼ 0.6 arcsec/pixel resolutions.
