Chandra Rules Out Super-Eddington Accretion Models for Little Red Dots
BibTeX Entry
@article{2025ApJ...989L..30S,
author = {{Sacchi}, Andrea and {Bogd{\'a}n}, {\'A}kos},
title = {{Chandra Rules Out Super-Eddington Accretion Models for Little Red Dots}},
journal = {\apjl},
keywords = {Accretion, Supermassive black holes, James Webb Space Telescope, Active galactic nuclei, X-ray active galactic nuclei, 14, 1663, 2291, 16, 2035, Astrophysics of Galaxies, Cosmology and Nongalactic Astrophysics, High Energy Astrophysical Phenomena},
year = {2025},
month = aug,
volume = {989},
number = {2},
eid = {L30},
pages = {L30},
doi = {10.3847/2041-8213/adf5c8},
archiveprefix = {arXiv},
eprint = {2505.09669},
primaryclass = {astro-ph.GA},
adsurl = {https://ui.adsabs.harvard.edu/abs/2025ApJ...989L..30S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
lrdkeys = {black hole mass, dust, early universe, jwst, x-ray},
month_numeric = {8}
}
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