AGN outflows are integral for understanding how the central super massive black hole interacts with the host galaxy and co-evolves in cosmic time. This white paper sets the primary science goals for the next decade and suggests the key parameters on which the next generation X-ray telescopes should be built to revolutionize our understanding.
The physics and astrophysics of X-ray outflows from Active Galactic Nuclei / Laha, ; Sibasish, ; Smith, ; Randall, ; Tzanavaris, ; Panayiotis, ; Kallman, ; Tim, ; Veilleux, ; Sylvain, ; Tombesi, ; Francesco, ; Kriss, ; Gerard, ; Guainazzi, ; Matteo, ; Gaspari, M; Kaastra, ; Jelle, ; Markowitz, ; Alex, ; Crenshaw, ; Mike, ; Behar, ; Ehud, ; Fukumura, ; Keigo, ; Longinotti, ; Anna, Lia; Rozanska, ; Agata, ; Ebrero, ; Jacobo, ; Ferland, ; Gary, ; Ricci, ; Claudio, ; Done, ; Chris, Proga; Daniel, ; Revalski, ; Mitchell, ; Vayner, ; Andrey,. - In: BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY. - ISSN 2330-9458. - 51:3(2019).
The physics and astrophysics of X-ray outflows from Active Galactic Nuclei
GASPARI M;
2019
Abstract
AGN outflows are integral for understanding how the central super massive black hole interacts with the host galaxy and co-evolves in cosmic time. This white paper sets the primary science goals for the next decade and suggests the key parameters on which the next generation X-ray telescopes should be built to revolutionize our understanding.
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