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Mildly Super-Eddington Accretion Onto Slowly-Spinning Bla... | ResearchHub
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Mildly Super-Eddington Accretion Onto Slowly-Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots
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Authors
Fabio Pacucci
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Fabio Pacucci
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Ramesh Narayan
Published
October 9, 2024
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Topics
Astrophysics
Materials Science
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DOI
10.3847/1538-4357/ad84f7
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arXiv License
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Preprint Server
Topics
Astrophysics
Materials Science
Computer Science
Physics
Optics
Show all topics
DOI
10.3847/1538-4357/ad84f7
License
arXiv License
