Disk Winds and the Accretion--Outflow Connection

dc.creatorKonigl, Arieh
dc.creatorPudritz, Ralph E.
dc.date1999-03-11
dc.date.accessioned2026-07-07T02:30:47Z
dc.date.available2026-07-07T02:30:47Z
dc.descriptionWe review recent observational and theoretical results on the relationship between circumstellar accretion disks and jets in young stellar objects. We then present a theoretical framework that interprets jets as accretion-powered, centrifugally driven winds from magnetized accretion disks. Recent progress in the numerical simulation of such outflows is described. We also discuss the structure of the underlying magnetized protostellar disks, emphasizing the role that large-scale, open magnetic fields can play in angular momentum transport.
dc.description32 pages, 3 figures, TeX, to appear in Protostars and Planets IV, ed. V. Mannings, A. Boss, and S. Russell (Arizona: University of Arizona Press)
dc.identifierhttps://arxiv.org/abs/astro-ph/9903168
dc.identifierhttp://arxiv.org/abs/astro-ph/9903168
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13936
dc.subjectAstrophysics
dc.titleDisk Winds and the Accretion--Outflow Connection
dc.typetext

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