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We analysed the ionised gas kinematics of the dwarf galaxy NGC 4214 usinghigh resolution Fabry-Perot interferometry observations and present a set ofnarrowband images in the H$\alpha$, [SII] $\lambda$6717 $\r{A}$, [NII]$\lambda$6584 $\r{A}$ and [OIII] $\lambda$5007 $\r{A}$ emission lines. Thehigh-resolution Fabry-Perot observations of the H$\alpha$ emission line,allowed us to derive the velocity field, the velocity dispersion $\sigma$, andthe rotation curve of the galaxy. We also present for the first time,three-dimensional kinematic maps of the complexes NGC 4214-I and NGC 4214-IIand analysed the kinematics of the ionised gas of two new superbubbles, as wellas the supernova remnants previously detected in this galaxy by other authors,in radio, optical and X-ray emission. We computed the expansion velocities ofthe superbubbles and supernova remnants fitting their velocity profiles andobtained their respective physical parameters. We found that the superbubbleshave an expansion velocity of ~50 km s$^{-1}$, dynamical age about $\sim$2 Myrand wind luminosity L$_W$ of ~9X10$^{38}$ erg s$^{-1}$ produced probably bymassive stars in OB associations. For supernova remnants, their expansionvelocities are between $\sim$48 to $\sim$80 km s$^{-1}$ with ages of about10$^{4}$ years and kinetic energy of about 10$^{51}$ erg assuming they are inthe radiative phase of evolution.

H$\alpha$ Kinematics of Superbubbles and Supernova Remnants of the Dwarf galaxy NGC 4214