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Title:
Ab initio simulations of accretion disc boundary layers
Authors:
Armitage, P. J.
Affiliation:
AA(University of St Andrews, School of Physics and Astronomy, North Haugh, Fife KY16 9SS, UK)
Publication:
The Physics of Cataclysmic Variables and Related Objects, ASP Conference Proceedings, Vol. 261. Edited by B. T. Gänsicke, K. Beuermann, and K. Reinsch. ISBN: 1-58381-101-X. San Francisco: Astronomical Society of the Pacific, 2002, p. 425.
Publication Date:
01/2002
Origin:
AUTHOR
Comment:
ISBN: 1-58381-101-X
Bibliographic Code:
2002ASPC..261..425A

Abstract

I discuss the results of simplified three dimensional magnetohydrodynamic simulations of the boundary layer between a disc and a non-rotating, unmagnetized star. Strong magnetic fields, possibly approaching equipartition with the thermal energy, occur in the boundary layer due to the shearing of disc-generated fields. The mean boundary layer magnetic field, which is highly variable on an orbital timescale, is estimated to exceed ~50 kG for a CV with an accretion rate of 10-9 Modot yr-1. However, these fields do not drive efficient angular momentum transport within the boundary layer. As a consequence the radial velocity in the boundary layer is low, and the density high.

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