RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries

In this study of the `Resolving supermAssive Black hole Binaries In galacTic hydrodynamical Simulations' (RABBITS) series, we focus on the hardening and coalescing process of supermassive black hole (SMBH) binaries in galaxy mergers. For simulations including different galaxy formation processe...

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Veröffentlicht in:	arXiv.org 2024-02
Hauptverfasser:	Liao, Shihong, Irodotou, Dimitrios, Johansson, Peter H, Naab, Thorsten, Rizzuto, Francesco Paolo, Hislop, Jessica M, Rawlings, Alexander, Wright, Ruby J
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Binary stars Coalescing Cooling Deposition Eccentricity Feedback Fixing Galactic evolution Galaxy mergers & collisions Gas cooling Gravitational waves Hardening Physics - Astrophysics of Galaxies Rabbits Simulation Star & galaxy formation Star formation Supermassive black holes Time measurement Torque
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