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The bound origin of low-mass stellar binaries

astro-ph.SR · 2026-05-15 · unverdicted · novelty 6.0

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 astro-ph.SR · 2026-05-15 · unverdicted · none · ref 34

    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.