Radiation-hydrodynamic Models of the Evolving Circumstellar Medium around Massive Stars

Details Radiation-hydrodynamic Models of the Evolving Circumstellar Medium around Massive Stars Radiation-hydrodynamic Models of the Evolving Circumstellar Medium around Massive Stars

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aspc..425..233t&link_type=abstract

Hot and Cool: Bridging Gaps in Massive Star Evolution ASP Conference Series Vol. 425, Proceedings of a Workshop held at the Cali

Astronomy and Astrophysics

Astronomy

Scientific paper

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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