Little Red Dots

Overview

  • Compact, extremely luminous infrared sources detected in the high-redshift early universe ().
  • Initial identifications emerged from jwst observations beginning in 2022.
  • Exhibit spectral energy distributions peaking in the red/infrared with flux densities inconsistent with standard galaxy evolution models.

Properties & Characteristics

  • Morphology: Highly compact structures; angular sizes comparable to distant quasars but lacking clear active galactic nucleus signatures in initial optical bands.
  • Luminosity: Intense emission suggesting high mass-accretion rates or exotic energy sources.
  • Spectral Features: Red spectral slope indicative of significant dust attenuation or specific emission mechanisms distinct from Population III stars.

Formation Models & Recent Evidence

References