Modified models of radiation pressure instability applied to 10, 105, and 107 M⊙ accreting black holes

Open Access

Fig. 15.

Dependence on the amplitude of the outburst (top panel) and the duration of the limit cycle (lower panel) of the accretion disk and magnetic coefficient b′ for black hole masses of 10 M_⊙ (left panel), 10⁵ M_⊙ (middle panel), and 10⁷ M_⊙ (right panel).

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