3D radiative hydrodynamic simulations of a 1.47-solar-mass F star show rotation-induced radius decrease, differential rotation, meridional flows, and latitude-dependent roll-like convection.
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Properties of Turbulent Convection and Large-Scale Flows in a Rotating F-type Star Revealed by 3D Realistic Radiative Hydrodynamic Simulations
3D radiative hydrodynamic simulations of a 1.47-solar-mass F star show rotation-induced radius decrease, differential rotation, meridional flows, and latitude-dependent roll-like convection.