Supermassive Black Hole Winds in X-rays: SUBWAYS

Context. Most active galactic nuclei (AGNs) are radio quiet (RQ), with radio emission that may arise from star-formation activity, AGN-driven winds, weak jets, and coronal activity. Disentangling these mechanisms is challenging and requires detailed multi-wavelength investigations, but it is crucial...

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Principais autores:	Amenta E., Brienza M., Bruni G., Brusa M., Morganti R., Panessa F., Baldi R. D., Behar E., Lanzuisi G., Shimwell T., Tombesi F., Bianchi S., Chartas G., Comastri A., Cresci G., De Marco B., Fiore F., Gaspari M., Gianolli V. E., Gilli R., Kraemer S. B., Kriss G., Krongold Y., La Franca F., Longinotti A. L., Mehdipour M., Nardini E., Perna M., Petrucci P., Piconcelli E., Ponti G., Ricci F., Zappacosta L.
Format:	Artigo
Jezik:	Inglês
Izdano:	EDP Sciences 2026-06-01
Serija:	Astronomy & Astrophysics
Teme:	instrumentation: interferometers methods: observational ism: jets and outflows galaxies: active galaxies: evolution radio continuum: galaxies
Online dostop:	https://www.aanda.org/articles/aa/full_html/2026/06/aa58621-25/aa58621-25.html
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