activity
19982025
most citedDynamical evolution of star clusters in tidal fields

775 citations · 12.1k across the 141 of their papers we have counts for

collaborators

142 papers

astro-ph.GA2025★ 4 cited

Direct N-body simulations of NGC 6397 and its tidal tails

Anthony D. Arnold, Holger Baumgardt

We have performed a series of direct N-body simulations that study the evolution of the Galactic globular cluster NGC 6397 under the combined influence of two-body relaxation, stel…

astro-ph.GA2023

The influence of black holes on the binary population of the globular cluster Palomar 5

Long Wang, Mark Gieles, Holger Baumgardt +3

The discovery of stellar-mass black holes (BHs) in globular clusters (GCs) raises the possibility of long-term retention of BHs within GCs. These BHs influence various astrophysica…

astro-ph.GA2023★ 3 cited

Multimass modelling of Milky Way globular clusters -- II. present-day black hole populations

Nolan Dickson, Peter J. Smith, Vincent Hénault-Brunet +2

Populations of stellar-mass black holes (BHs) in globular clusters (GCs) influence their dynamical evolution and have important implications on one of the main formation channels f…

astro-ph.GA2023★ 1 cited

Testing QUMOND theory with Galactic globular clusters in a weak external field

A. Sollima, C. Nipoti, F. Calura +2

We developed self-consistent dynamical models of stellar systems in the framework of quasi-linear modified Newtonian dynamics (QUMOND). The models are constructed from the anisotro…

astro-ph.GA2023★ 23 cited

Multimass modelling of Milky Way globular clusters -- I. Implications on their stellar initial mass function above 1 M

Nolan Dickson, Vincent Hénault-Brunet, Holger Baumgardt +2

The distribution of stars and stellar remnants (white dwarfs, neutron stars, black holes) within globular clusters holds clues about their formation and long-term evolution, with i…

astro-ph.SR2023★ 2 cited

Multiple stellar populations at less evolved stages-III: a possible helium spread in NGC 2210

Chengyuan Li, Xin Ji, Long Wang +6

Helium variations are common features of globular clusters (GCs) with multiple stellar populations. All the formation scenarios predict that secondary population stars are enhanced…