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AGN in Clumpy DisCs (ACDC): How does ISM structure shape multiphase outflows?

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If you have a question about this talk, please contact Sandro Tacchella .

In this talk, I will present our simulations of an AGN wind embedded within a spatially-resolved, clumpy ISM to reveal the effect of ISM structure on the propagation of AGN -driven outflows. I will also discuss the observational implications of this work, for example, in the construction of AGN -galaxy scaling relations, and how can we observationally constrain whether an outflow is energy or momentum driven.

This talk is part of the Galaxies Discussion Group series.

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