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Investigating the origin of radio emission in candidate super-Eddington accreting black holes

Context. Recent studies show that the radio power of quasars accreting at very high rates can reach surprisingly high values. These studies suggest that this radio emission could originate from star formation (SF); however, the lack of data does not rule out the presence of a jetted active galactic...

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Detaylı Bibliyografya
Asıl Yazarlar: Gendron-Marsolais M., Marziani P., Berton M., Järvelä E., del Olmo A., Sargent M., D’Onofrio M., Crepaldi L., Damas-Segovia A., Punsly B., Verdes-Montenegro L.
Materyal Türü: Artigo
Dil:Inglês
Baskı/Yayın Bilgisi: EDP Sciences 2026-03-01
Seri Bilgileri:Astronomy & Astrophysics
Konular:
Online Erişim:https://www.aanda.org/articles/aa/full_html/2026/03/aa57025-25/aa57025-25.html
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