Gravitational torque-driven black hole growth and feedback in cosmological simulations

By Daniel Anglés-Alcázar, R. Dav'e, C. Faucher-Giguére, F. Özel, P. F. H. Northwestern, U. Cape, Arizona, Caltech. 2016

156 citations recorded by the source corpus.

CIERA Postdoctoral Fellowship; South African Research Chairs Initiative; South African National Research Foundation; NASA ATP grant [NNX12AH86G, NNX14AH35G]; NSF [AST-1412836, AST-1517491, AST-1108753, 1411920, 1455342, ACI-1053575, PHY-1066293]; NASA [NNX15AB22G]; STScI [HST-AR-14293.001-A, HST-GO-14268.022-A]; NASA TCAN award [NNX14AB48G]; Alfred P. Sloan Research Fellowship

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/8ae69e519ed1217742db7a664329ae1eb2bcc106

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Citations in the corpus

simba: Cosmological simulations with black hole growth and feedback (2019, methodology): “In previous works, Anglés-Alcázar et al. (2015) and Anglés-Alcázar et al. (2017a) showed that the MBH − M∗ relation emerged naturally from the torque-limited accretion model, without or with AGN feedback, respectively.”
Black holes on FIRE: stellar feedback limits early feeding of galactic nuclei (2017, background): “Dwarf galaxies experience bursty star formation down to z = 0 (e.g. Anglés-Alcázar et al. 2017b), suggesting that BH growth will also be inefficient in low-redshift dwarfs.”
The Romulus cosmological simulations: a physical approach to the formation, dynamics and accretion models of SMBHs (2016, methodology): “This creates a more physical picture of how, when, and where SMBHs grow compared to the more common Bondi-Hoyle prescription, while avoiding the additional assump- tions and free parameters required by other current methods (e.g. Rosas-Guevara et al. 2015; Anglés-Alcázar et al. 2017).”
Supermassive black holes and their feedback effects in the IllustrisTNG simulation (2017, background): “…simulations of representative cosmological volumes (Vogelsberger et al. 2014; Schaye et al. 2015; Dubois et al. 2016; Khandai et al. 2015; Anglés-Alcázar et al. 2017b; Tremmel et al. 2017b) it is possible to track the evolution of SMBHs and their host galaxies through cosmic time and…”
Galaxy Interactions Trigger Rapid Black Hole Growth: an unprecedented view from the Hyper Suprime-Cam Survey (2017, background): “…to be subject to substantial gravitational torques, resulting in the efficient loss of angular momentum, ultimately causing substantial gas flow towards the BH, and igniting a powerful AGN (e.g., Barnes & Hernquist 1991; Mihos & Hernquist 1996; Di Matteo et al. 2008; Anglés-Alcázar et al. 2017).”
AGN outflows and feedback twenty years on (2018, unknown): “Crucially, such approaches also reproduce the scaling relations between black hole mass and host properties (see also [24]).”