Fig. 2

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Population A: atmospheric mass loss undergone by Magrathea gas giants, scattered in the mass-distance parameter space. The x-axis corresponds to the final time-averaged orbital distance of the CBPs. We show the planets that lost more mass than the 50% of the category. The colour corresponds to the amount of mass lost (see colour bar). The size of the markers is proportional to the progenitor binary mass, as illustrated in the legend.
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