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Fig. 2
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Differences between the three considered cases, ∆(1−3)rM(rorb), ∆(1−2)rM(rorb), and ∆(2−3)rM(rorb), following Eqs (19)–(21). The blue (orange) dots represent planets orbiting the inner (outer) radii of the HZ. The results for the slow wind are given on the panels on the left, the results for the fast wind on the right.
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