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20232026
most citedDynamical evolution of Milky Way globular clusters on the cosmological timescale I. Mass loss and interaction with the nuclear star cluster

11 citations · 22 across the 4 of their papers we have counts for

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5 papers · 1 filter

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.GA20261 cited

How our proto-nuclear star cluster formed and grew due to early globular cluster disruption. I. Case of low masses

D. Kuvatova, M. Ishchenko, P. Berczik +3

We investigate the accretion of globular cluster stars on early cosmological timescales through detailed N-body simulations of theoretical GC models to assess the role of this mech…

astro-ph.GA202411 cited

Dynamical evolution of Milky Way globular clusters on the cosmological timescale I. Mass loss and interaction with the nuclear star cluster

M. Ishchenko, P. Berczik, T. Panamarev +7

Context. Based on the Gaia DR3, we reconstructed the orbital evolution of the known Milky Way globular clusters and found that six objects, NGC 6681, NGC 6981, Palomar 6, NGC 6642,…

astro-ph.GA202310 cited

Milky Way globular clusters on cosmological timescales. III. Interaction rates

Maryna Ishchenko, Margaryta Sobolenko, Peter Berczik +4

Aims. We carry out the self-consistent dynamic evolution of the orbital structure of Milky Way globular clusters. This allows us to estimate possible and probable close passages an…

astro-ph.GA202325 cited

Milky Way globular clusters on cosmological timescales. I. Evolution of the orbital parameters in time-varying potentials

M. Ishchenko, M. Sobolenko, P. Berczik +4

Context. Recent observational data show that the Milky Way (MW) galaxy contains about 170 globular clusters (GCs). A fraction of them is likely formed in dwarf galaxies accreted on…