Black hole mergers from dwarf to massive galaxies with the NewHorizon and Horizon-AGN simulations

Massive black hole (MBH) coalescences are powerful sources of low-frequency gravitational waves. To study these events in the cosmological context, we need to trace the large-scale structure and cosmic evolution of a statistical population of galaxies, from dim dwarfs to bright galaxies. To cover su...

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Bibliographic Details
Main Authors: Volonteri, M, Pfister, H, Beckmann, RS, Dubois, Y, Colpi, M, Conselice, CJ, Dotti, M, Martin, G, Jackson, R, Kraljic, K, Pichon, C, Trebitsch, M, Yi, SK, Devriendt, J, Peirani, S
Format: Journal article
Language:English
Published: Oxford University Press 2020