Searching for clues of past binary supermassive black hole mergers in nuclear star clusters

Author(s)
Alessandra Mastrobuono-Battisti, Go Ogiya, Oliver Hahn, Mathias Schultheis
Abstract

Galaxy mergers are common processes in the Universe. As a large fraction of galaxies hosts at their centres a central supermassive black hole (SMBH), mergers can lead to the formation of a supermassive black hole binary (SMBHB). The formation of such a binary is more efficient when the SMBHs are embedded in a nuclear star cluster (NSC). NSCs are dense and massive stellar clusters present in the majority of the observed galaxies. Their central densities can reach up to 107, Mpc-3 and their masses can be as large as a few 107M. The direct detection of an SMBHB is observationally challenging. In this work, we illustrate how the large-scale structural and dynamical properties of an NSC can help to identify nucleated galaxies that recently went through a merger that possibly led to the formation of a central SMBHB. Our models show that the merger can imprint signatures on the shape, density profile, rotation, and velocity structure of the NSC. The strength of the signatures depends on the mass ratio between the SMBHs and on the orbital initial conditions of the merger. In addition, the number of hypervelocity stars produced in the mergers is linked to the SMBHB properties. The merger can also contribute to the formation of the nuclear stellar disc of the galaxy.

Organisation(s)
Department of Astrophysics, Department of Mathematics
External organisation(s)
Université Côte d'Azur, Université de recherche Paris Sciences et Lettres, Zhejiang University (ZJU), University of Waterloo (UW)
Journal
Monthly Notices of the Royal Astronomical Society
Volume
521
Pages
6089-6104
No. of pages
16
ISSN
0035-8711
DOI
https://doi.org/10.1093/mnras/stad898
Publication date
03-2023
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Keywords
ASJC Scopus subject areas
Astronomy and Astrophysics, Space and Planetary Science
Portal url
https://ucrisportal.univie.ac.at/en/publications/808742a7-5b2b-4709-b070-1d0737fc3f78