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20062026
most citedDynamics of Planetary Systems in Star Clusters

159 citations · 196 across the 11 of their papers we have counts for

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Showing astro-ph.GAShow all

10 papers · 1 filter

astro-ph.GA2026

The evolution of high-z proto-star clusters into local globular clusters

A. Della Croce, E. Vesperini, R. Pascale +4

The James Webb Space Telescope (JWST) detected numerous massive and relatively compact stellar clumps around proto-galaxies at high redshift (z>0.5). Their properties suggest that…

astro-ph.GA2026

Massive star clusters detected by JWST as natural birth places to form intermediate-mass black holes

Dominik R. G. Schleicher, Matías Liempi, Mirek Giersz +11

The James Webb Space Telescope (JWST) has detected, through gravitational lensing, several young massive star clusters (YMCs), which are considered as relevant building blocks of h…

astro-ph.GA2026

Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problem

P. Berczik, O. Sobodar, F. Flammini Dotti +5

Recent observations indicate that in some Milky Way globular clusters (GCs) pristine red giant branch (RGB) stars appear more centrally concentrated than enriched ones. This contra…

astro-ph.GA2025★ 6 cited

Evolution of star clusters with initial bulk rotation via N-body simulations

Abylay Bissekenov, Xiaoying Pang, Albrecht Kamlah +6

Young star clusters can inherit bulk rotation from the molecular clouds from which they have formed. This rotation can affect the long-term evolution of a star cluster and its cons…

astro-ph.GA2025★ 16 cited

Rapid formation of a very massive star >50000 and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters

Marcelo C. Vergara, Abbas Askar, Albrecht W. H. Kamlah +15

Context. We present simulations of a massive young star cluster using \textsc{Nbody6++GPU} and \textsc{MOCCA}. The cluster is initially more compact than previously published model…

astro-ph.GA2024★ 10 cited

Energy equipartition in multiple-population globular clusters

A. R. Livernois, F. I. Aros, E. Vesperini +7

We present the results of Monte Carlo simulations aimed at exploring the evolution towards energy equipartition of first- (1G) and second-generation (2G) stars in multiple-populati…