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Interaction Of A Stellar Magnetic Field With A Turbulent Accretion Disk

Published online by Cambridge University Press:  12 April 2016

Anne Bardou  and
Jean Heyvaerts
Anne Bardou
Affiliation:
Observatoire de Strasbourg, 11 rue de l’Université, 67000 Strasbourg, France
Jean Heyvaerts
Affiliation:
Observatoire de Strasbourg, 11 rue de l’Université, 67000 Strasbourg, France

Abstract

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Magnetized objects surrounded by a turbulent and keplerian accretion disk are considered. In such systems, magnetic field lines are embedded into the disk. The magnetic field of the central object is assumed to be dipolar in the absence of the accretion disk. In the presence of a turbulent accretion disk, it is shown that the interaction with the disk stretches magnetic field lines along the disk and that most of the non-magnetospheric magnetic flux is expelled outside the disk.

Type
Part 5. Magnetic Fields and Viscosity
Information
International Astronomical Union Colloquium , Volume 163: Accretion Phenomena and Related Outflows , 1997 , pp. 205 - 209
Copyright
Copyright © Astronomical Society of the Pacific 1997

References

Aly, J.J. 1984, ApJ, 283, 349 CrossRefGoogle Scholar
Aly, J.J. 1991, ApJ, 375, L61 CrossRefGoogle Scholar
Bardou, A., Heyvaerts, J. 1996, A&A, 307, 1009 Google Scholar
Lynden-Bell, D., Boily, C. 1994, MNRAS, 267, 146 CrossRefGoogle Scholar