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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 3.

Observed versus model-predicted FWHMs of the broad-line component. Both kinetic and scattering effects are taken into account when calculating the velocity dispersion. The dashed line marks the 1:1 relation.

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