Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots
BibTeX Entry
@article{2026arXiv260717448L,
author = {{Liu}, Jun-Rong and {Feng}, Hua and {Ho}, Luis C.},
title = {{Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots}},
journal = {arXiv e-prints},
keywords = {High Energy Astrophysical Phenomena, Astrophysics of Galaxies},
year = {2026},
month = jul,
eid = {arXiv:2607.17448},
pages = {arXiv:2607.17448},
archiveprefix = {arXiv},
eprint = {2607.17448},
primaryclass = {astro-ph.HE},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026arXiv260717448L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
month_numeric = {7}
}
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