Fig. 7.
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Thermal solutions of the MAD numerical simulation for an XRB with MBH = 10 M⊙ at two different radii of r = 8 rg (solid lines) and r = 3 rg (dashed lines). The gray lines show the hot, optically thin branches, and the gold lines show the cold, optically thick branches. The inner radii can stay hot to higher ṁ than the outer radii.
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