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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 0.1-0.4, 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.
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Monthly Notices of the Royal Astronomical Society
University of Cambridge
University of Leicester
Space Telescope Science Institute
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