posted on 2012-10-24, 09:06authored byA. R. King, J. E. Pringle, M. Livio
We consider observational and theoretical estimates of the accretion disc viscosity parameter α. We find that in thin, fully ionized discs, the best observational evidence suggests a typical range α∼ 0.1–0.4, whereas the relevant numerical simulations tend to derive estimates for α which are an order of magnitude smaller. We discuss possible reasons for this apparent discrepancy.
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Citation
Monthly Notices of the Royal Astronomical Society, 2007, 376 (4), pp. 1740-1746