Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters

ABSTRACT Using the SWIFT simulation code, we compare the effects of different forms of active galactic nuclei (AGNs) feedback in idealized galaxy groups and clusters. We first present a physically motivated model of black hole (BH) spin evolution and a numerical implementation of thermal isotropic f...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2024-01, Vol.527 (3), p.5988-6020
Hauptverfasser:	Huško, Filip, Lacey, Cedric G, Schaye, Joop, Nobels, Folkert S J, Schaller, Matthieu
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Astronomical models Black holes Feedback Galactic clusters Galaxies Quenching Star & galaxy formation Star formation Wind effects
Online-Zugang:	Volltext
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