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Radiative hydrodynamics simulations of red supergiant stars

Radiative hydrodynamics simulations of red supergiant stars

Context. The red supergiant (RSG) Betelgeuse is an irregular variable star. Convection may play an important role in understanding this variability. Interferometric observations can be interpreted using sophisticated simulations of stellar convection. Aims. We compare the visibility curves and closure phases obtained from our 3D simulation of RSG convection with …