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I briefly mention our ongoing studies and the recent results of the ionized gas kinematics in several nearby irregular galaxies. Because of their thick disk, large gas reservour and a lack of spiral density waves, irregular galaxies are an ideal laboratory to study the effects of the massive stars and young star clusters feedback on ISM. Here I focus on two aspects of our studies - searching and analyzing of superbubbles in ISM and the study of the unique stellar objects, which significantly influence on ISM.