Super-Eddington outflows from 10^5–10^7 M_sun black holes, with 3000–6000 K photospheres, can account for Little Red Dots' red continua, broad-line widths, and Balmer breaks.
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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots
Super-Eddington outflows from 10^5–10^7 M_sun black holes, with 3000–6000 K photospheres, can account for Little Red Dots' red continua, broad-line widths, and Balmer breaks.