Astro2020 Science White Paper: Do Supermassive Black Hole Winds Impact Galaxy Evolution?. (arXiv:1903.07664v1 [astro-ph.HE])
<a href="http://arxiv.org/find/astro-ph/1/au:+Tombesi_F/0/1/0/all/0/1">F. Tombesi</a> (1, 2, 3, 4), <a href="http://arxiv.org/find/astro-ph/1/au:+Cappi_M/0/1/0/all/0/1">M. Cappi</a> (5), <a href="http://arxiv.org/find/astro-ph/1/au:+Carrera_F/0/1/0/all/0/1">F. Carrera</a> (6), <a href="http://arxiv.org/find/astro-ph/1/au:+Chartas_G/0/1/0/all/0/1">G. Chartas</a> (7), <a href="http://arxiv.org/find/astro-ph/1/au:+Fukumura_K/0/1/0/all/0/1">K. Fukumura</a> (8), <a href="http://arxiv.org/find/astro-ph/1/au:+Guainazzi_M/0/1/0/all/0/1">M. Guainazzi</a> (9), <a href="http://arxiv.org/find/astro-ph/1/au:+Kazanas_D/0/1/0/all/0/1">D. Kazanas</a> (2), <a href="http://arxiv.org/find/astro-ph/1/au:+Kriss_G/0/1/0/all/0/1">G. Kriss</a> (10), <a href="http://arxiv.org/find/astro-ph/1/au:+Proga_D/0/1/0/all/0/1">D. Proga</a> (11), <a href="http://arxiv.org/find/astro-ph/1/au:+Turner_T/0/1/0/all/0/1">T. J. Turner</a> (12), <a href="http://arxiv.org/find/astro-ph/1/au:+Ueda_Y/0/1/0/all/0/1">Y. Ueda</a> (13), <a href="http://arxiv.org/find/astro-ph/1/au:+Veilleux_S/0/1/0/all/0/1">S. Veilleux</a> (1), <a href="http://arxiv.org/find/astro-ph/1/au:+Brusa_M/0/1/0/all/0/1">M. Brusa</a> (14, 5), <a href="http://arxiv.org/find/astro-ph/1/au:+Gaspari_M/0/1/0/all/0/1">M. Gaspari</a> (15) ((1) University of Maryland, College Park, (2) NASA/GSFC, (3) University of Rome Tor Vergata, (4) INAF-OAR, (5) INAF-OAS, (6) Istituto de Fisica de Cantabria, (7) College of Charleston, (8) James Madison University, (9) ESA, (10) Space Telescope Science Institute, (11) University of Nevada, Las Vegas, (12) University of Maryland, Baltimore County, (13) Kyoto University, (14) University of Bologna, (15) Princeton University)
Powerful winds driven by supermassive black holes (SMBHs) are likely the main
mechanism through which SMBHs regulate their own growth and influence the host
galaxy evolution. However, their origin and their capability to impact the
large-scale environment are still highly debated. Fundamental results will come
from high-energy and spatial resolution X-ray observatories.
Powerful winds driven by supermassive black holes (SMBHs) are likely the main
mechanism through which SMBHs regulate their own growth and influence the host
galaxy evolution. However, their origin and their capability to impact the
large-scale environment are still highly debated. Fundamental results will come
from high-energy and spatial resolution X-ray observatories.
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