Dynamical dissolution of soft primordial binaries fully explains observed main-sequence binary fractions in globular clusters under solar-neighborhood initial conditions.
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N-body simulations find that primordial mass segregation imprints denser, unified tidal tails with bottom-heavy mass functions on star clusters, with effects strongest early and at small R_G but converging later.
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An analytical approach to binary populations in globular clusters
Dynamical dissolution of soft primordial binaries fully explains observed main-sequence binary fractions in globular clusters under solar-neighborhood initial conditions.
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The fingerprint of primordial mass segregation on the tidal tails of star clusters
N-body simulations find that primordial mass segregation imprints denser, unified tidal tails with bottom-heavy mass functions on star clusters, with effects strongest early and at small R_G but converging later.