Modelling the Accretion on Young Stars, Recent Results and Perspectives

L. de Sá,C. Stehlé, J. P. Chièze,I. Hubeny,T. Lanz,S. Colombo, L. Ibgui,S. Orlando

HAL (Le Centre pour la Communication Scientifique Directe)（2018）

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摘要

Despite intense observational work, the stellar accretion process is insufficiently constrained, and consequently the details in the exchange of mass and momentum between the proto-star and its accretion disk remain approximate.

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young stars,accretion

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