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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Next-generation IFU instruments could detect core scouring and tangential anisotropy from MBH binaries up to z~0.14 for ~150 pc cores and higher redshifts for larger cores, expanding searchable volume by 30-40 times including lower-mass systems.
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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.
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Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP
Next-generation IFU instruments could detect core scouring and tangential anisotropy from MBH binaries up to z~0.14 for ~150 pc cores and higher redshifts for larger cores, expanding searchable volume by 30-40 times including lower-mass systems.