Hydrodynamical simulations of Milky Way-like cluster formation find that most binaries are bound from formation, half are disrupted by the end of the star-formation epoch, and multiple formation accounts for at least 57% of stars.
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The bound origin of low-mass stellar binaries
Hydrodynamical simulations of Milky Way-like cluster formation find that most binaries are bound from formation, half are disrupted by the end of the star-formation epoch, and multiple formation accounts for at least 57% of stars.