Fig. 3.
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Top: Amount of mass accreted over time by the MBH in our Stellar Feedback simulations (see Table 2). Dashed lines indicate the percentage growth of an initial 104 M⊙ MBH. Bottom: Corresponding time evolution of the MBH gas accretion rate (in terms of the Eddington fraction fEdd = ṀBH/ṀEdd). Transparent background lines correspond to the obtained gas accretion rate of individual snapshots, while opaque lines mark the running mean value over 20 Myr.
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