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, M., Nagai, D., Zhuravleva, I., Brummel-Smith, C., Li, Y., Hodges-Kluck, E., Yang, H.K., Basu, K., Chluba, J., Churazov, E., Donahue, M., Fabian, A., Faucher-Giguère, C., Gaspari, M., Hlavacek-Larrondo, J., Mcdonald, M., Mcnamara, B., Nulsen, P., Mroczkowski, T., Mushotzky, R., et al.. - In: BULLETIN OF THE AMERICAN ASTRONOMICAL SOCIETY. - ISSN 2330-9458. - 51:3(2019), p. 326.
Supermassive Black Hole Feedback
GASPARI, MASSIMO;
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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