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Tracing AGN feedback, from the SMBH horizon up to cluster scales

Published online by Cambridge University Press:  29 January 2021

Francesco Tombesi
Francesco Tombesi*
Affiliation:
Department of Physics, University of Rome ‘Tor Vergata’, Via della Ricerca Scientifica 1, I-00133 Rome, Italy INAF Astronomical Observatory of Rome, Via Frascati 33, 00078 Monte Porzio Catone, Italy Department of Astronomy, University of Maryland, College Park, MD 20742, USA NASA/Goddard Space Flight Center, Code 662, Greenbelt, MD 20771, USA
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Abstract

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Observations performed in the last decades have shown that supermassive black holes (SMBHs) and cosmic structures are not separate elements of the Universe. While galaxies extend on spatial scales about ten orders of magnitude larger than the horizon of SMBHs, black holes would not exist without matter feeding them, and cosmic structures would not be the same without feedback from SMBHs. Powerful winds/jets in active galactic nuclei (AGN) may be the basis of this co-evolution. Synergistic observations in the X-rays and other wavebands have been proven to be fundamental to map AGN winds from the event horizon up to galaxy scales, providing a promising avenue to study the multi-phase SMBH feeding and feedback processes. Moreover, a spatially resolved, spectroscopic analysis of AGN in clusters will allow us to probe the multiphase medium ranging from galactic up to cluster scales. Revolutionary advances are expected in the upcoming decade with new multi-wavelength observatories, ranging from radio to X-rays.

Keywords

Active galactic nucleisupermassive black holesAGN feedbackX-ray astronomyAGN winds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S356: Nuclear Activity in Galaxies Across Cosmic Time , October 2019 , pp. 218 - 222
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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