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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Published in | Astronomy and astrophysics (Berlin) Vol. 599; p. A86 |
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Main Authors | , , |
Format | Journal Article |
Language | English |
Published |
EDP Sciences
01.03.2017
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Subjects | |
Online Access | Get full text |
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