Abstract
Winds and jets of T Tauri stars are generated in the inner part of the accretion disk around protostellar objects. The interaction between a magnetized protostellar object and its accretion disk generates magnetized disk winds, which are collimated on a scale of ≃ 50 AU. The magnetic structure of these disk winds follows from the self-consistent solutions of the force-balance equation. Stationary solutions of the relativistic Grad-Schlüter-Shafranov (GSS) equation with different field topologies applied to a protostellar star-disk system are presented
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© 1994 Springer Science+Business Media Dordrecht
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Fendt, C., Camenzind, M. (1994). Wind Magnetospheres of Protostellar Accretion Disks. In: Duschl, W.J., Frank, J., Meyer, F., Meyer-Hofmeister, E., Tscharnuter, W.M. (eds) Theory of Accretion Disks — 2. NATO ASI Series, vol 417. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0858-4_5
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DOI: https://doi.org/10.1007/978-94-011-0858-4_5
Publisher Name: Springer, Dordrecht
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