Magnetic Interaction between Stars and Accretion Disks
arXiv:astro-ph/0310104 · doi:10.1023/B:ASTR.0000045064.93078.87
Abstract
In this review I consider modern theoretical models of coupled star--disk magnetospheres. I discuss a number of models, both stationary and time-dependent, and examine what physical conditions govern the selection of a preferred model.
Invited review at the International Workshop on Magnetic Fields in Star Formation (Madrid, April 21--25, 2003)