Ruszkowski, MateuszMateuszRuszkowskiNagai, DaisukeDaisukeNagaiZhuravleva, IrinaIrinaZhuravlevaBrummel-Smith, CoreyCoreyBrummel-SmithLi, YuanYuanLiHodges-Kluck, EdmundEdmundHodges-KluckYang, Hsiang-Yi KarenHsiang-Yi KarenYangBasu, KaustuvKaustuvBasuChluba, JensJensChlubaChurazov, EugeneEugeneChurazovDonahue, MeganMeganDonahueFabian, AndrewAndrewFabianFaucher-Giguère, Claude-AndréClaude-AndréFaucher-GiguèreGASPARI, MASSIMOMASSIMOGASPARIHlavacek-Larrondo, JulieJulieHlavacek-LarrondoMcDonald, MichaelMichaelMcDonaldMcNamara, BrianBrianMcNamaraNulsen, PaulPaulNulsenMroczkowski, TonyTonyMroczkowskiMushotzky, RichardRichardMushotzkyReynolds, ChristopherChristopherReynoldsVikhlinin, AlexeyAlexeyVikhlininVoit, MarkMarkVoitWerner, NorbertNorbertWernerZuHone, JohnJohnZuHoneZweibel, EllenEllenZweibel2020-12-292020-12-2920192330-9458http://hdl.handle.net/20.500.12386/29269Galaxy 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.ELETTRONICOenArticlehttps://baas.aas.org/pub/2020n3i326/release/12019BAAS...51c.326RFIS/05 - ASTRONOMIA E ASTROFISICA