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Fig. 8

image

Left: influence of the gas giant’s orbital and physical parameters. Top and bottom subpanels are for a secondary F-type and M-type star, respectively. Right: the three subpanels show results for the case of single star systems. Each plot corresponds to an intermediate integration time of 10 Myr. See text in Sect. 5 and legend of Fig. 6 for more details.

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