Fig. 5

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Spin alignment process in the idealised Milky Way galaxy. Top panels: angle subtended by the BH angular momentum and the z-axis θr. Bottom panels: BH spin parameter a. Quantities are plotted as a function of time (left panels) and of the ratio between accreted and initial BH mass MBH/MBH,0 (right). Each line represents one simulation of the set summarised in Table 1. Dotted lines represent the instant after which condition (6) is no longer satisfied.
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