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Structure and evolution of circumstellar shells formed by massive star winds
Authors:Guillermo García-Segura  Mordecai-Mark Mac Low  Norbert Langer
Institution:(1) Instituto de Astrofísica de Canarias, University of Illinois, Urbana-Champaign, USA;(2) University of Chicago, Urbana-Champaign, USA;(3) University of Illinois, Urbana-Champaign, USA;(4) Max-Planck-Institut für Astrophysik, Garching, Germany
Abstract:We follow the interaction of massive stars with their circumstellar gas over their entire life-times by combining hydrodynamic stellar evolution calculations for 35 and 60M odot stars and one- and two-dimensional gas dynamical calculations for the circumstellar medium.
Keywords:massive stars  mass loss  LBV-nebulae  WR nebulae
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