3D hydrodynamic simulations of massive main-sequence stars. III. The effect of radiation pressure and diffusion leading to a 1D equilibrium model
Huaqing Mao(Hubei University of Arts and Science), Paul R. Woodward(University of Minnesota), Falk Herwig, Pavel A. Denissenkov, W. T. Thompson(Goddard Space Flight Center), Simon Blouin(Los Alamos National Laboratory)
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