arXiv Open Access 2012

Feedback from Winds and Supernovae in Massive Stellar Clusters

Julian Pittard Hazel Rogers

Lihat Sumber

Abstrak

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.

Topik & Kata Kunci

astro-ph.GA astro-ph.SR

Penulis (2)

Julian Pittard

Hazel Rogers

Format Sitasi

APA MLA BibTeX

Pittard, J., Rogers, H. (2012). Feedback from Winds and Supernovae in Massive Stellar Clusters. https://arxiv.org/abs/1209.5276

Akses Cepat

Lihat di Sumber

Informasi Jurnal

Tahun Terbit: 2012
Bahasa: en
Sumber Database: arXiv
Akses: Open Access ✓