AGN wind scaling relations and the co-evolution of black holes and galaxies
By Fabrizio Fiore, C. Feruglio, F. Shankar, M. Bischetti, A. Bongiorno, M. Brusa, S. Carniani, C. Cicone, F. Duras, A. Lamastra and 7 more. 2017
338 citations recorded by the source corpus.
This work was supported by ASI/INAF contract I/009/10/0 and INAF PRIN 2011, 2012 and 2014. MB acknowledges support from the FP7 Career Integration Grant “eEASy” (CIG 321913). LZ acknowledges support from ASI/INAF grant I/037/12/0. CF acknowledges funding from the European Union Horizon 2020 research and innovation programme under the Marie SklodowskaCurie grant agreement No 664931. CC acknowledges funding from the European Union Horizon 2020 research and innovation programme under the Marie SklodowskaCurie grant agreement No 664931 and support from Swiss National Science Foundation Grants PP00P2 138979 and PP00P2 166159. RM acknowledges the ERC Advanced Grant 695671 QUENCH and support from the Science and Technology Facilities Council (STFC).
Subfields: Astronomy and Astrophysics
View Paper: https://www.semanticscholar.org/paper/6c038b9c2c452bda6f67f5f6419c29a31455f25e
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Citations in the corpus
- simba: Cosmological simulations with black hole growth and feedback (2019, background): “MNRAS 000, 1–25 (2018) Based on observations of AGN outflows and the inferred momentum and energy input (e.g. Fiore et al. 2017; Ishibashi et al. 2018), we set the amount of material ejected in the AGN winds in order to obtain a momentum input of ÛPout = 20 L/c, where L = η ÛMBH c2 is the…”
- First results from the TNG50 simulation: galactic outflows driven by supernovae and black hole feedback (2019, background): “Many of the observational data points in this regime, for instance of the Fiore et al. (2017) compilation, are thought to be black hole driven outflows.”
- AGN outflows and feedback twenty years on (2018, positive): “In most cases these different approaches give similar values of vout within a factor of a few or better[33, 46].”