collaborators

9 papers

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.GA2026

Dynamical evolution of Milky Way globular clusters on the cosmological timescale II. Terzan 2, 4, and 5 mass loss and collision tracking

M. Ishchenko, P. Berczik, D. Kuvatova

We investigate the long-term dynamical evolution of Ter2, Ter4, and Ter5, focusing on their mutual interactions, mass-loss behaviour, and survivability in the dense Galactic centre…

astro-ph.GA2026

Global m=1 slow mode in near-Keplerian self-gravitating torus: applications to stellar nuclear disks and AGN molecular tori

Elena Bannikova, Volodymyr Akhmetov, Peter Berczik +3

Global m=1 asymmetries are observed in many self-gravitating astrophysical systems and are often interpreted as large-scale slow modes in near-Keplerian potentials. Prominent examp…

astro-ph.GA2026

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.GA2025

Globular clusters of the Gaia Enceladus/Sausage -- I. Orbital and dynamical evolution on cosmological timescales

Mykyta Bilodid, Maryna Ishchenko, Peter Berczik

We investigated Gaia-Enceladus/Sausage globular cluster samples and studied their orbital and dynamical evolution over cosmological timescales in external time-variable potential.…

astro-ph.GA2025

Dynamical evolution timescales for the supermassive black hole system in the galaxy NGC 7727 (Arp 222)

P. Berczik, M. Ishchenko, O. Veles +5

Context. A dual active galactic nucleus candidate with a separation of only 500 pc was recently found in NGC 7727. According to the hierarchical merging scenario, such objects woul…