J. Bouvier
Published 2013-10-16Version 1
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.
Comments: Summary talk, 4 pages, to appear in the Proceedings of "Physics at the Magnetospheric Boundary", Geneva, 25-28 June 2013
[Fe II] 1.64 um Features of Jets and Outflows from Young Stellar Objects in the Carina Nebula
Variability of Ha emission in young stellar objects in the cluster IC 348
Radio Jets from Young Stellar Objects
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