Fig. 7
Dependence between period and amplitude of flares for a stellar-mass black hole (M = 10 M⊙, upper panel), an intermediate-mass black hole (M = 3 × 104M⊙, middle panel), and a supermassive black hole (M = 108M⊙, lower panel). Computations were made for a range of μ but values for a different μ lie predominantly along the main correlation trend resulting in a very low scatter.
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