Three-body encounters in black hole discs around a supermassive black hole: The disc velocity dispersion and the Keplerian tidal field determine the eccentricity and spin-orbit alignment of gravitational wave mergers

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  • aa47920-23

    Final published version, 792 KB, PDF document

Original languageEnglish
Article numberA135
JournalAstronomy & Astrophysics
Volume683
Number of pages12
ISSN0004-6361
DOIs
Publication statusPublished - 15 Mar 2024

ID: 389304723