Pyroclastic Blowout: Dust Survival in Isolated versus Clustered Supernovae
Following the current debate on the fate of SN-condensed dust grains, here we explore by means of three-dimensional hydrodynamical simulations the interaction of dusty supernova remnants (SNRs) with the shocked winds of neighboring massive stars within young massive stellar clusters (SSCs). As a comparison, we have also explored the evolution of
Martínez-González, S. et al.
Fecha de publicación:
10
2018