Accretion disc viscosity: how big is alpha?
arXiv:astro-ph/0701803 · doi:10.1111/j.1365-2966.2007.11556.x
Abstract
We consider observational and theoretical estimates of the accretion disc viscosity parameter . We find that in thin, fully-ionized discs, the best observational evidence suggests a typical range , whereas the relevant numerical simulations tend to derive estimates for which are an order of magnitude smaller. We discuss possible reasons for this apparent discrepancy.
MNRAS, in press