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3D Hydrodynamic Simulations of Massive Main-sequence Stars. III. The Effect of Radiation Pressure and Diffusion Leading to a 1D Equilibrium Model - IOPscienceSearchopens in new tabopens in new tab
3D Hydrodynamic Simulations of Massive Main-sequence Stars. III. The Effect of Radiation Pressure and Diffusion Leading to a 1D Equilibrium Model, Mao, Huaqing, Woodward, Paul, Herwig, Falk, Denissenkov, Pavel A., Blouin, Simon, Thompson, William, McDermott, Benjamin