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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 4.

Distribution of Balmer break strengths in LRDs. The shaded region shows the expected range from the fiducial outflow model with M = 106 M⊙ and ﹩\dot{m}=2000﹩ given a covering factor from 0.1 (left side) to 0.8 (right side).

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