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Origins of the UV Continuum and Balmer Emission Lines in Little Red Dots: Observational Validation of Dense Gas Envelope Models Enshrouding the Active Galactic Nucleus

  • Authors: Yoshihisa Asada, Kohei Inayoshi, Qinyue Fei, Seiji Fujimoto, Chris J. Willott

Yoshihisa Asada et al 2026 The Astrophysical Journal Letters 1005 .

  • Provider: AAS Journals

Caption: Figure 4.

Lyα line equivalent widths of the sample broad Hα emitters at z = 5–7.2, plotted against the rest-UV absolute magnitude. They distribute at a very similar locus as normal SFGs at the same redshift range (J. Kerutt et al. 2022), and there is no significant difference between LRDs and LBDs.

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