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.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
fields
astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Test-particle simulations show that Galactic bar pattern speed systematically deflects open-cluster tidal tail orientations, with NGC 2632 and Hyades tails disfavouring moderate speeds.
citing papers explorer
-
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.
-
Bar-induced deflection of open cluster tidal tails
Test-particle simulations show that Galactic bar pattern speed systematically deflects open-cluster tidal tail orientations, with NGC 2632 and Hyades tails disfavouring moderate speeds.