The <scp>dragon-II</scp> simulations – III. Compact binary mergers in clusters with up to 1 million stars: mass, spin, eccentricity, merger rate, and pair instability supernovae rate

This is a publication. If there is no link to the publication on this page, you can try the pre-formated search via the search engines listed on this page.

Authors: Manuel Arca sedda; Albrecht W H Kamlah; Rainer Spurzem; Francesco Paolo Rizzuto; Mirek Giersz; Thorsten Naab; Peter Berczik

Journal title: Monthly Notices of the Royal Astronomical Society

Journal publisher: Blackwell Publishing Inc.

Published year: 2024

DOI identifier: 10.1093/mnras/stad3951

ISSN: 0035-8711