Abstract
Abstract We discuss a number of topics relevant to disk-magnetosphere interaction and how numerical simulations illuminate them. The topics include: (1) disk-magnetosphere interaction and the problem of disk-locking; (2) the wind problem; (3) structure of the magnetospheric flow, hot spots at the star's surface, and the inner disk region; (4) modeling of spectra from 3D funnel streams; (5) accretion to a star with a complex magnetic field; (6) accretion through 3D instabilities; (7) magnetospheric gap and survival of protoplanets. Results of both 2D and 3D simulations are discussed.
| Original language | English |
|---|---|
| Pages (from-to) | 277-290 |
| Number of pages | 14 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 3 |
| Issue number | 1 S243 |
| DOIs | |
| State | Published - Aug 2007 |
Keywords
- Accretion
- Accretion disks
- Stars: early-type
- Stars: magnetic fields
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