Fig. A.8
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Population B. Shown are the stellar types of the inner binaries for those planets that do not become Magratheas. From left to right: CBPs around merging binaries, excluded the DWD-mergers, planets in the Collided and Destabilised categories (see Sect. 4 for the detailed definitions). For simplicity, the label ‘Post-MS’ includes all the stellar types after the MS that are not WDs.
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