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Feedback from Winds and Supernovae in Massive Stellar Clusters

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 نشر من قبل Julian Pittard
 تاريخ النشر 2012
  مجال البحث فيزياء
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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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