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University of Cambridge > Talks.cam > Galaxies Discussion Group > AGN in Clumpy DisCs (ACDC): How does ISM structure shape multiphase outflows?
AGN in Clumpy DisCs (ACDC): How does ISM structure shape multiphase outflows?Add to your list(s) Download to your calendar using vCal
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. This talk is included in these lists:
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