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| Paper: |
Radiation-hydrodynamic Models of the Evolving Circumstellar Medium around Massive Stars |
| Volume: |
425, Hot and Cool: Bridging Gaps in Massive Star Evolution |
| Page: |
233 |
| Authors: |
Toal\’ a, J. A.; Arthur, S. J. |
| Abstract: |
We present the results of time-dependent, radiation-hydrodynamic models of the evolving circumstellar medium around stars with initial masses of 40 and 60 Msun. Our models show the difference that the assumption of a rotating star can make to the resulting circumstellar medium, which is principally due to the difference in length of the intense mass-loss stages. We model the formation of structure due to instabilities in the cold shell-fast wind interaction region. |
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