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Intermediate-mass stripped stars in the Magellanic Clouds: Forward modeling the observed population discovered via UV excess
Stripped stars are hot, helium-rich stars formed when binary interactions remove a star’s hydrogen envelope. While low-mass (≲1 M⊙) and high-mass (≳8 M⊙) stripped stars are well studied as hot subdwarfs and Wolf–Rayet stars, their intermediate-mass counterparts (1–8 M⊙) have only recently been disco
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