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Fig. 9


Fraction of incoming water in the HZ with respect to the initial total amount of water in the disk of planetesimals, considering various configurations. Top and middle panels show results in binary star systems for fixed and variable values of the gas giant’s orbital and physical parameters, respectively, when the secondary is an F-type (left) and M-type (right) star (see text in Sect. 5.1). Comparison with various single star systems are shown in the bottom panel (see text in Sect. 5.2).

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