The purpose of the StarAcc project is to improve the understanding and modeling of accretion columns in magnetic binary systems by combining theoretical and numerical studies, experimental and observational studies. It proposes an original and unprecedented approach to the phenomena of shock accretion and irradiation, relying in particular on the use of power lasers. It is particularly focused on the study of radiative instabilities developing in the accretion flow channeled by the magnetic field
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Dernière mise à jour : Nov 19th, 2024
