Abstract
La nature de l'interaction dans la couche limite entre un disque d'accretion et l'etoile centrale est etudiee. Des criteres simples sont etablis afin d'estimer la profondeur dans l'etoile pour laquelle l'interaction disque-etoile se developpe de maniere significative. Ces criteres sont appliques a une variete de systemes de disques d'accretion et les consequences observationnelles pour les variables cataclysmiques et les etoiles de type T Tauri sont discutees
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