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.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

© 2006-2024 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity