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Fig. 8.


Time evolution of model 14. Bottom panel: transition radius (black curve) as well as the outer disc radius (red curve). Top panel: actual mass accretion rate (black curve) and critical rate (green curve). The blue curve gives the analytic solutions (Eq. (13)) when the entire disc is in the hot state, and the red curve corresponds to a propagating cooling front (Eq. (22)).

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