Simulating galaxy formation with black hole driven thermal and kinetic feedback
© 2016 The Authors. The inefficiency of star formation in massive elliptical galaxies is widely believed to be caused by the interactions of an active galactic nucleus (AGN) with the surrounding gas. Achieving a sufficiently rapid reddening of moderately massive galaxies without expelling too many b...
Main Authors: | Weinberger, Rainer (Author), Springel, Volker (Author), Hernquist, Lars (Author), Pillepich, Annalisa (Author), Marinacci, Federico (Author), Pakmor, Rüdiger (Author), Nelson, Dylan (Author), Genel, Shy (Author), Vogelsberger, Mark (Author), Naiman, Jill (Author), Torrey, Paul A. (Author) |
---|---|
Other Authors: | Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor) |
Format: | Article |
Language: | English |
Published: |
Oxford University Press (OUP),
2022-07-22T14:42:54Z.
|
Subjects: | |
Online Access: | Get fulltext |
Similar Items
-
Simulating galaxy formation with black hole driven thermal and kinetic feedback
by: Weinberger, Rainer, et al.
Published: (2021) -
Ejective and preventative: the IllustrisTNG black hole feedback and its effects on the thermodynamics of the gas within and around galaxies
by: Zinger, Elad, et al.
Published: (2021) -
A Quantification of the Butterfly Effect in Cosmological Simulations and Implications for Galaxy Scaling Relations
by: Genel, Shy, et al.
Published: (2021) -
Submillimetre galaxies in cosmological hydrodynamical simulations - an opportunity for constraining feedback models
by: Hayward, Christopher C, et al.
Published: (2022) -
The fraction of dark matter within galaxies from the IllustrisTNG simulations
by: Lovell, Mark R., et al.
Published: (2019)