Numerical simulations of continuum-driven winds of super-Eddington stars

We present the results of numerical simulations of continuum-driven winds of stars that exceed the Eddington limit and compare these against predictions from earlier analytical solutions. Our models are based on the assumption that the stellar atmosphere consists of clumped matter, where the individ...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2008-09, Vol.389 (3), p.1353-1359
Hauptverfasser:	Van Marle, A. J., Owocki, S. P., Shaviv, N. J.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Astrophysics Earth, ocean, space Exact sciences and technology Fluid dynamics hydrodynamics Mathematical models methods: numerical outflows Stars & galaxies stars: mass-loss stars: winds stars: winds, outflows Wind
Online-Zugang:	Volltext
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