activity
20122026
most citedAn iterative method for the construction of N-body galaxy models in collisionless equilibrium

102 citations · 207 across the 8 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

5 papers · 1 filter

astro-ph.GA2025

Taming the plunge: A circularization trap of supermassive black hole binaries

Pau Amaro Seoane, Alessandra Mastrobuono Battisti, Chingis Omarov +5

We investigate the orbital eccentricity evolution of supermassive black hole binaries within galactic environments. We analyze the dynamics in triaxial merger remnants and subseque…

astro-ph.GA2024

Prograde and retrograde stars in nuclear cluster mergers. Evolution of the supermassive black hole binary and the host galactic nucleus

Alessandra Mastrobuono-Battisti, Pau Amaro Seoane, Màrius Josep Fullana i Alfonso +5

We address the orbital distribution of stars in merging nuclear star clusters (NSCs) and the subsequent effects on supermassive black hole binary (SMBHB) evolution. We ran direct-s…

astro-ph.GA2023★ 10 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.GA2022★ 7 cited

Intermediate-mass ratio inspirals in merging elliptical galaxies

Verónica Vázquez-Aceves, Pau Amaro Seoane, Dana Kuvatova +3

Close encounters between two initially unbound objects can result in a binary system if enough energy is released as gravitational waves (GWs). We address the scenario in which suc…

astro-ph.GA2014★ 53 cited

The stability of stellar disks in Milky-Way sized dark matter halos

Denis Yurin, Volker Springel

We employ an improved methodology to insert live stellar disks into high-resolution dark matter simulations of Milky Way sized halos, allowing us to investigate the fate of thin st…