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arxiv: astro-ph/9903168 · v1 · pith:HC5DHA3N · submitted 1999-03-11 · astro-ph

Disk Winds and the Accretion--Outflow Connection

Arieh Konigl (University of Chicago) , Ralph E. Pudritz (McMaster University) This is my paper

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keywords disksaccretionjetsmagnetizedrecenttheoreticalwindsaccretion--outflow
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We 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.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. GeV {\gamma}-ray emission in the low-mass star-forming region AFGL 490

    astro-ph.HE 2026-05 unverdicted novelty 6.0

    Discovery of extended GeV gamma-ray emission from AFGL 490, with the protostellar jet identified as the likely particle accelerator rather than stellar winds.