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| Paper: |
Feedback from Winds and Supernovae in Massive Stellar Clusters |
| Volume: |
465, Four Decades of Massive Star Research - A Scientific Meeting in Honor of Anthony J. Moffat |
| Page: |
398 |
| Authors: |
Pittard, J. M.; Rogers, H. |
| Abstract: |
We simulate the effects of massive star feedback, via winds and
SNe, on inhomogeneous molecular material left over from the formation
of a massive stellar cluster. We use 3D hydrodynamic models
with a temperature dependent average particle mass to model the
separate molecular, atomic, and ionized phases. We find that the
winds blow out of the molecular clump along low-density channels, and
gradually ablate denser material into these. However, the dense molecular gas
is surprisingly long-lived and is not immediately affected by the
first star in the cluster exploding. |
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