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.
H., Haghi H., K \"u pper A
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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.