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2006MNRAS.368..379M - Mon. Not. R. Astron. Soc., 368, 379-396 (2006/May-1)
Variability of black hole accretion discs: the cool, thermal disc component.
MAYER M. and PRINGLE J.E.
Abstract (from CDS):
We are now better placed to put physical constraints on model parameters. In particular, we find that in order to be consistent with the low degree of variability seen in the thermal disc component of black hole binaries, we need to limit the energy density of the poloidal field that can be produced by local dynamo cells in the disc to less than a few per cent of the energy density of the dynamo field within the disc itself.
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): black hole physics - galaxies: jets - X-rays: binaries
Simbad objects: 10
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