Photon scattering 3D radiation-hydrodynamical simulations of late-type stellar atmospheres
Numerical models of stellar atmospheres fulfill an important role in astrophysical research. They describe the physical environment from which stellar radiation originates, allowing detailed analyses of the temperature and pressure stratification in the atmosphere, of the chemical composition, atmospheric motion, phenomena related to magnetic fields and more. Theoretical studies of stellar atmospheres usually involve two steps: first, the model atmosphere is constructed according to a set of...[Show more]
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