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Structured outflow from a dynamo active accretion disc
Uppsala University, Teknisk-naturvetenskapliga vetenskapsområdet, Physics, Department of Astronomy and Space Physics.
2003 (English)In: Astronomy & Astrophysics, Vol. 398, no 3, 825-844 p.Article in journal (Refereed) Published
Abstract [en]

We present an axisymmetric numerical model of a dynamo active accretion disc. If the dynamo-generated magnetic field in the disc is sufficiently strong (close to equipartition with thermal energy), a fast magneto-centrifugally driven outflow develops

Place, publisher, year, edition, pages
2003. Vol. 398, no 3, 825-844 p.
Identifiers
URN: urn:nbn:se:uu:diva-47871OAI: oai:DiVA.org:uu-47871DiVA: diva2:75778
Available from: 2008-10-17 Created: 2008-10-17 Last updated: 2011-01-13

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