Dusty Supernovae within Superbubbles
Sergio Martínez González
I will present our hydrodynamical modelling of the injection and survival of the dust grains produced by sequential supernovae. Our goal has been to investigate whether supernovae are net producers or destroyers of interstellar dust. We have found that they indeed lead to massively enhance the amount of dust within low-metallicity star-forming molecular clouds, in accordance with the large dust masses present in galaxies soon after the onset of cosmic reionization.
Location: Sporilov, 101