One-zone models for spheroidal galaxies with a central supermassive black-hole - Self-regulated Bondi accretion

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Fig. 1

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The self-regulated Bondi accretion rate obtained from Eq. (31) is represented by the heavy solid line. The dotted line is the accretion rate determined by Eq. (25). Note how for very low and very high classical accretion rates Ṁ_B, the two prescriptions coincide.

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