A unified accretion model reveals an effectively optically thin, radiation-pressure-supported flow between the standard thin disk and slim disk, producing a multi-color Wien spectrum and constraining viscosity to alpha ~ 0.03.
https://ui.adsabs.harvard.edu/abs/1977A&A....59..127C 59
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The effectively optically thin accretion flow and its implication in supermassive black holes
A unified accretion model reveals an effectively optically thin, radiation-pressure-supported flow between the standard thin disk and slim disk, producing a multi-color Wien spectrum and constraining viscosity to alpha ~ 0.03.