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Three Dimensional Radiation Hydrodynamic Simulations of Massive Star Envelopes
Yan-Fei Jiang, Matteo Cantiello, Lars Bildsten +3
(Abridged) Stars more massive than are so luminous that the radiation force on the cooler, more opaque outer layers can balance or exceed the force of gravity. The…
Convection Enhances Magnetic Turbulence in AM CVn Accretion Disks
Matthew S. B. Coleman, Omer Blaes, Shigenobu Hirose +1
We present the results of local, vertically stratified, radiation magnetohydrodynamic shearing box simulations of magnetorotational instability (MRI) turbulence for a (hydrogen poo…
The Effects of Magnetic Fields on the Dynamics of Radiation Pressure Dominated Massive Star Envelopes
Yan-Fei Jiang, Matteo Cantiello, Lars Bildsten +2
We use three dimensional radiation magneto-hydrodynamic simulations to study the effects of magnetic fields on the energy transport and structure of radiation pressure dominated ma…
Local Radiation Hydrodynamic Simulations of Massive Star Envelopes at the Iron Opacity Peak
Yan-Fei Jiang, Matteo Cantiello, Lars Bildsten +2
We perform three dimensional radiation hydrodynamic simulations of the structure and dynamics of radiation dominated envelopes of massive stars at the location of the iron opacity…