Galaxy evolution is critically shaped by the energy injection from supermassive black holes (SMBHs). A major challenge is unraveling how the energy released near the SMBHs is distributed throughout galaxies and their environments. This white paper discusses the prospect of tackling this problem using high-resolution X-ray/microwave observations.
Supermassive Black Hole Feedback / Ruszkowski, ; Mateusz, ; Nagai, ; Daisuke, ; Zhuravleva, ; Irina, ; Brummel-Smith, ; Corey, ; Li, ; Yuan, ; Hodges-Kluck, ; Edmund, ; Yang, ; Hsiang-Yi, Karen; Basu, ; Kaustuv, ; Chluba, ; Jens, ; Churazov, ; Eugene, ; Donahue, ; Megan, ; Fabian, ; Andrew, ; Faucher-Giguère, ; Claude-André, ; Gaspari, M; Hlavacek-Larrondo, ; Julie, ; Mcdonald, ; Michael, ; Mcnamara, ; Brian, ; Nulsen, ; Paul, ; Mroczkowski, ; Tony, ; Mushotzky, ; Richard, Reynolds; Christopher, ; Vikhlinin, ; Alexey, ; Voit, ; Mark, ; Werner, ; Norbert, ; Zuhone, ; John, ; Zweibel, ; Ellen,. - In: BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY. - ISSN 2330-9458. - 51:3(2019).
Supermassive Black Hole Feedback
GASPARI M;
2019
Abstract
Galaxy evolution is critically shaped by the energy injection from supermassive black holes (SMBHs). A major challenge is unraveling how the energy released near the SMBHs is distributed throughout galaxies and their environments. This white paper discusses the prospect of tackling this problem using high-resolution X-ray/microwave observations.
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