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, K., Basu, ., Kaustuv, ., Chluba, ., Jens, ., Churazov, ., Eugene, ., et al.. - 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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