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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 5.

Distribution of Balmer decrements in LRDs. The shaded region shows the expected range from the outflow model with M and ﹩\dot{m}﹩ determined from the observed luminosity and temperature for each object.

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