Spiral-driven accretion in protoplanetary discs III. Tridimensional simulations

Context. Understanding how accretion proceeds in proto-planetary discs, and more generally, understanding their dynamics, is a crucial questions that needs to be answered to explain the conditions in which planets form. Aims. The role that accretion of gas from the surrounding molecular cloud onto t...

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Bibliographic Details
Published inAstronomy and astrophysics (Berlin) Vol. 599; p. A86
Main Authors Hennebelle, Patrick, Lesur, Geoffroy, Fromang, Sébastien
Format Journal Article
LanguageEnglish
Published EDP Sciences 01.03.2017
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