Mildly Super-Eddington Accretion Onto Slowly-Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots

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Bibliographic Details
Main Authors:	Pacucci, Fabio, Narayan, Ramesh
Format:	Preprint
Published:	2024
Subjects:	High Energy Astrophysical Phenomena Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Online Access:	Acceder al recurso
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Internet

https://arxiv.org/abs/2407.15915