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Optically Thick Outflow Driven by Supercritical Accretion May Explain Little Red Dots

  • Authors: Jun-Rong Liu, Hua Feng, Luis C. Ho

Jun-Rong Liu et al 2026 The Astrophysical Journal Letters 1007 .

  • Provider: AAS Journals

Caption: Figure 2.

Blackbody luminosity versus temperature measured from the red envelope in LRDs (circles) and the local analog “The Egg” (star). The dashed and dotted lines show the predicted blackbody luminosity and temperature from the outflow model at different black hole masses (M = 105, 106, and 107 M) and accretion rates (﹩\dot{m}=1500﹩, 3000, and 5000).

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