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.
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Uzdensky, D.A. (2004). Magnetic Interaction Between Stars and Accretion Disks. In: de Castro, A.I.G., Heyer, M., Vázquez-Semadeni, E., Rebolo, R., Tagger, M., Pudritz, R.E. (eds) Magnetic Fields and Star Formation. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-0491-5_41
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DOI: https://doi.org/10.1007/978-94-017-0491-5_41
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