Represented on the y-axis (left and right axes have the same scale), the variation of the maximum eccentricity (red line) together with the cumulative fraction of water (dashed black line) brought to the HZ, with respect to the initial location of small bodies in ℛ2 and ℛ3. The top panel is for a secondary star at qb = 35 au and the bottom panel is for qb = 45 au. In this figure, is also represented the normalized HZc distribution (blue line) from 0.1 Myr (left) up to 50 Myr (right). The vertical black line refers to the position of the snow line. The entire region ℛ3 is intentionally not displayed because of its size. Instead, only the dynamically interesting part of ℛ3 is shown.
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