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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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Bibliografski detalji
Glavni autori: 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.
Format: Artigo
Jezik:Inglês
Izdano: EDP Sciences 2026-03-01
Serija:Astronomy & Astrophysics
Teme:
Online pristup:https://www.aanda.org/articles/aa/full_html/2026/03/aa57025-25/aa57025-25.html
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