Virtually all massive galaxies, including our own, host central black holes ranging in mass from millions to billions of solar masses. The growth of these black holes releases vast amounts of energy that powers quasars and other weaker active galactic nuclei. A tiny fraction of this energy, if absorbed by the host galaxy, could halt star formation by heating and ejecting ambient gas. A central question in galaxy evolution is the degree to which this process has caused the decline of star formation in large elliptical galaxies, which typically have little cold gas and few young stars, unlike spiral galaxies.
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A.C. thanks his wife A. Fylaktou for assistance in making the Review readable for a broader audience.
Author Contributions A.C. initiated the project, wrote the first draft, and had editorial control throughout. He chose to have many co-authors to show that the Review reflects consensus within the field. S.M.F. made a major contribution to the structure and content of the Review. J.B., A.D., J.K. and R.M. participated extensively in the writing of the manuscript, A.B., P.B., and M.B. contributed significantly to individual sections. A.K., A.M. and P.B. produced Figs 2, 3 and 4, respectively. The other authors contributed mainly by providing comments on drafts and by participating in scientific discussions in connection with: X-ray observations of galaxy clusters (A.C.F.), galaxy formation (C.S.F., M.S.), the interaction of radiation with the interstellar medium (H.N.), the interaction of quasar winds with the interstellar medium (J.S.), and quasar winds and host galaxies (L.W.).
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Cattaneo, A., Faber, S., Binney, J. et al. The role of black holes in galaxy formation and evolution. Nature 460, 213–219 (2009). https://doi.org/10.1038/nature08135
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