Hostname: page-component-8448b6f56d-c4f8m Total loading time: 0 Render date: 2024-04-24T09:52:46.515Z Has data issue: false hasContentIssue false
  • English
  • Français

Stellar wind and supernova feedback from massive stars

Published online by Cambridge University Press:  05 March 2015

Julian M. Pittard  and
Hazel Rogers
Julian M. Pittard
Affiliation:
School of Physics and Astronomy, The University of Leeds, Leeds, LS2 9JT, UK email: jmp@ast.leeds.ac.uk
Hazel Rogers
Affiliation:
School of Physics and Astronomy, The University of Leeds, Leeds, LS2 9JT, UK email: jmp@ast.leeds.ac.uk
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have constructed three-dimensional hydrodynamical models to simulate the impact of massive star feedback, via winds and SNe, on inhomogeneous molecular material left over from the formation of a massive stellar cluster. We are studying the timescales for the molecular material to be removed from the environment of a massive stellar cluster and the mass and energy fluxes into the wider environment.

Keywords

hydrodynamicsISM: bubblesHII regionssupernova remnants
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 10 , Highlights H16: Highlights of Astronomy , August 2012 , pp. 586
Copyright
Copyright © International Astronomical Union 2015