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The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The ultraviolet photometric catalog and stripped-star candidate selection
Most massive stars (∼8–25M⊙) interact with a binary companion during their lifetimes. These interactions can remove the hydrogen-rich envelope, producing intermediate-mass (∼2–8M⊙) and helium-rich stars. These “stripped stars” are predicted to emit predominantly in the ultraviolet (UV) and can there
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