Feedback in Galaxy Formation
arXiv:1102.0283 · doi:10.1017/S1743921311022939
Abstract
I review the outstanding problems in galaxy formation theory, and the role of feedback in resolving them. I address the efficiency of star formation, the galactic star formation rate, and the roles of supernovae and supermassive black holes.
To appear in the proceedings of IAU Symposium 277, Burkina Faso, December 2010, Tracing the Ancestry of Galaxies (on the Land of our Ancestors), C. Carignan, F. Combes \& K. Freeman, eds
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Cited by in corpus (4)
- Chemical Signatures of the First Galaxies: Criteria for One-Shot Enrichment
- The Effect of Environment on Type Ia Supernovae in the Dark Energy Survey Three-Year Cosmological Sample
- The failure of stellar feedback, magnetic fields, conduction, and morphological quenching in maintaining red galaxies
- Being KLEVER at cosmic noon: ionised gas outflows are inconspicuous in low-mass star-forming galaxies but prominent in massive AGN hosts