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Fig. 7.

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Two potential binary evolution pathways leading to the formation of a stripped star in SMCSGS-FS 69. The Case B mass transfer evolution roughly matches most of the derived surface properties, though it notably requires ≳40% accretion efficiency to reproduce the secondary (Fig. E.1). The Case A mass transfer evolution does not have that requirement, but it overpredicts the current mass of the stripped star.

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