Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots
BibTeX Entry
@article{2026ApJ..1007L..13L,
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 = {\apjl},
keywords = {Active galactic nuclei, Black holes, Accretion, 16, 162, 14},
year = {2026},
month = aug,
volume = {1007},
number = {1},
eid = {L13},
pages = {L13},
doi = {10.3847/2041-8213/ae8dba},
adsurl = {https://ui.adsabs.harvard.edu/abs/2026ApJ..1007L..13L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
dimensions = {true},
month_numeric = {8}
}
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