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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Autors principals:	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
Idioma:	Inglês
Publicat:	EDP Sciences 2026-06-01
Col·lecció:	Astronomy & Astrophysics
Matèries:	instrumentation: interferometers methods: observational ism: jets and outflows galaxies: active galaxies: evolution radio continuum: galaxies
Accés en línia:	https://www.aanda.org/articles/aa/full_html/2026/06/aa58621-25/aa58621-25.html
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