Late-time mass loss in low-mass helium-star binaries produces shock-cooling light curves that match a subset of fast, blue Type Ib/n supernovae and some fast blue optical transients.
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Shock cooling emission from late-time mass loss in low-mass He star binaries
Late-time mass loss in low-mass helium-star binaries produces shock-cooling light curves that match a subset of fast, blue Type Ib/n supernovae and some fast blue optical transients.