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Presentation #311.01 in the session “Star-forming Regions at Distant Galaxies”.
Over the last decade we have performed a series of spectroscopic and photometric studies of the kinematics and energetics of massive star formation, form the local example of 30 Dor to high redshift (z ~ 3). In this talk I will review our main findings on the star formation in the context of Super Star Clusters and its influence on the interstellar medium. I will argue that Super Star Clusters are an excellent laboratory to study the evolution of the Universe.