Mildly Super-Eddington Accretion onto Slowly Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots
BibTeX Entry
@article{2024ApJ...976...96P,
author = {{Pacucci}, Fabio and {Narayan}, Ramesh},
title = {{Mildly Super-Eddington Accretion onto Slowly Spinning Black Holes Explains the X-Ray Weakness of the Little Red Dots}},
journal = {\apj},
keywords = {Active galaxies, Supermassive black holes, Black holes, Accretion, Spectral energy distribution, 17, 1663, 162, 14, 2129, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - Astrophysics of Galaxies},
year = {2024},
month = nov,
volume = {976},
number = {1},
eid = {96},
pages = {96},
doi = {10.3847/1538-4357/ad84f7},
archiveprefix = {arXiv},
eprint = {2407.15915},
primaryclass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2024ApJ...976...96P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
altmetric = {165611420},
lrdkeys = {early universe, jwst, sed, simulation, x-ray},
month_numeric = {11}
}
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