Fig. 2
T and Σ variability for the model with μ = 0.5 for a typical IMBH accretion disk. The computation shows a weakly developed instability. Parameters: M = 3 × 104M⊙, α = 0.02, and ṁ = 0.25. The plot is made for the radius 
cm. The red curve represents the stationary model and the green dots show local values of the temperature for the time-dependent computation.
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