Stellar-feedback-driven outflows & galaxy formation

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Modern large-volume cosmological simulations rely on stellar feedback-driven outflows to solve the 'overcooling' problem, but they must incorporate such outflows via highly uncertain sub-resolution prescriptions. In contrast, state-of-the-art simulations with resolved stellar feedback generate outflows self-consistently. I will discuss the underlying physics of such outflows and describe how simulations and theoretical models for outflows can be tested using future radio/(sub)mm facilities.

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