Abstract
This summary talk aims at highlighting some of the remaining open issues regarding the physics of the magnetospheric accretion/ejection process in young stellar objects (YSOs). It lists a number of questions related to YSOs magnetic fields and accretion regimes, the structure and properties of accretion shocks, the origin of multiple outflow components, and the impact of the star-disk magnetic interaction onto early angular momentum evolution.
Highlights
The presentations at this conference have clearly illustrated the new insights theory, numerical simulations, and observations have brought to our understanding of the magnetic star-disk interaction process in young stellar objects (YSOs)
This summary talk aims at highlighting some of the remaining open issues regarding the physics of the magnetospheric accretion/ejection process in young stellar objects (YSOs)
It lists a number of questions related to YSOs magnetic fields and accretion regimes, the structure and properties of accretion shocks, the origin of multiple outflow components, and the impact of the star-disk magnetic interaction onto early angular momentum evolution
Summary
The presentations at this conference have clearly illustrated the new insights theory, numerical simulations, and observations have brought to our understanding of the magnetic star-disk interaction process in young stellar objects (YSOs). I shall rely on these presentations to outline in this summary talk some of the remaining issues to be addressed in the forthcoming years regarding the origin and properties of YSOs magnetic fields, the eventuality of different accretion regimes, the physics of accretion shocks, the coexistence of several outflow components, and their impact on angular momentum evolution
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