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Stellar feedback in the interstellar medium

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The interstellar medium drives galaxy formation and outflows. Its multi-phase structure is set by gravitation, cooling and chemistry as well as “feedback”, mostly form massive stars. I will present results from recent simulations with a well resolved interstellar medium and discuss the impact of stellar winds, ionising radiation, and supernova explosions on setting the ISM structure and the initial driving of galactic outflows.

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