activity
20162026
most citedStar-disc interaction in galactic nuclei: orbits and rates of accreted stars

72 citations · 274 across the 15 of their papers we have counts for

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Showing 2026Show all

6 papers · 1 filter

astro-ph.GA2026

Stellar discs and intermediate-mass black holes in galactic nuclei II. Fragmenting the disc and forming the S-stars in a live nuclear star cluster

Taras Panamarev, Bence Kocsis

We present direct -body simulations of a stellar disc around the supermassive black hole Sgr~A*, perturbed by an intermediate-mass black hole (IMBH) and embedded in a live nucle…

astro-ph.GA2026

Simulating tidal disruption events in nuclear star clusters

Philip Cho, Kai Wu, Francesco Flammini Dotti +5

Context. Nuclear star clusters (NSCs) and supermassive black holes (SMBHs) often coexist at the centers of galaxies, engaging in complex dynamical interactions that influence SMBH…

astro-ph.GA2026

Stellar discs and intermediate-mass black holes in galactic nuclei I. Fragmenting the disc in an isotropic stellar potential

Taras Panamarev, Xiang Zou, Bence Kocsis

The origin of the complex orbital structure of young massive stars at the Galactic centre remains an open question. If these stars formed in a single episode from a gaseous accreti…

astro-ph.HE2026

The contribution to Galactic Centre γ-ray excess from cluster-born millisecond pulsars. Constraints from direct N-body simulations

M. Kalambay, M. Ishchenko, D. Kuvatova +2

The Galactic Centre γ-ray excess (GCE), observed by Fermi-LAT around Sgr A*, exceeds expectations from standard cosmic-ray models and is commonly attributed either to dark matter a…

astro-ph.GA2026

Modeling Tidal Disruption Events and Compact Object Plunges in Nuclear Star Clusters

Philip Cho, Kai Wu, Francesco Flammini Dotti +2

We study tidal disruption events (TDEs) and compact object inspirals in nuclear star clusters (NSCs) hosting a central supermassive black hole (SMBH), focusing on their role in SMB…

astro-ph.GA2026★ 1 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…