101 citations · 171 across the 5 of their papers we have counts for
7 papers
Revealing the Formation of the Milky Way Nuclear Star Cluster via Chemo-Dynamical Modeling
Tuan Do, Gregory David Martinez, Wolfgang Kerzendorf +4
The Milky Way nuclear star cluster (MW NSC) has been used as a template to understand the origin and evolution of galactic nuclei and the interaction of nuclear star clusters with…
Fingerprints of binary black hole formation channels encoded in the mass and spin of merger remnants
Manuel Arca Sedda, Michela Mapelli, Mario Spera +2
Binary black holes (BBHs) are thought to form in different environments, including the galactic field and (globular, nuclear, young and open) star clusters. Here, we propose a meth…
Birth, life, and death of black hole binaries around supermassive black holes: dynamical evolution of gravitational wave sources
Manuel Arca Sedda
In this paper, we explore the mechanisms that regulate the formation and evolution of stellar black hole binaries (BHBs) around supermassive black holes (SMBHs). We show that dynam…
Mergers of globular clusters in the Galactic disc: intermediate mass black hole coalescence and implications for gravitational waves detection
Manuel Arca Sedda, Alessandra Mastrobuono-Battisti
We propose a new formation channel for intermediate mass black hole (IMBH) binaries via globular cluster collisions in the Galactic disc. Using numerical simulations, we show that…
The future Milky Way and Andromeda galaxy merger
Riccardo Schiavi, Roberto Capuzzo Dolcetta, Manuel Arca Sedda
According to our current knowledge about physical and dynamical properties of the Milky Way-M31 system, it seems likely that these two galaxies will collide and eventually merge in…
MOCCA-SURVEY Database I. Intermediate mass black holes in Milky Way globular clusters and their connection to supermassive black holes
Manuel Arca Sedda, Abbas Askar, Mirek Giersz
In this paper we explore the interplay between intermediate-mass black holes (IMBHs) and their nursing globular clusters (GCs), taking advantage of over 2000 Monte Carlo GC models.…