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Massive stars and the energy balance of the ISM: I. The imapct of an isolated 60 M starWe present results of numerical simulations carried out with a 2D radiation hydrodynamics code in order to study the impact of massive stars on their surrounding interstellar medium. This first paper deals with the evolution of the circumstellar gas around an isolated 60 M star.
Document ID
20060042533
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Yorke, H. W.
Freyer, T.
Hensler, G.
Date Acquired
August 23, 2013
Publication Date
January 1, 2002
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
galaxies evolution HII regions hydsodynamics interstellar medium