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Fig. 13.
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Same as Fig. 10 but for 2.80 M⊙ + NS binary systems. For comparison, the dashed orange line in panel c indicates the NS-NS merger fraction of ∼25% for the post-CE binary without any interactions, and around 44% of binaries merge within a Hubble time after binary MT (post-CE-MT), which is denoted by the dotted orange line.
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