The Astrophysical Journal Letters (Jan 2025)

Discovery of Local Analogs to JWST’s Little Red Dots

  • Ruqiu Lin,
  • Zhen-Ya Zheng,
  • Chunyan Jiang,
  • Fang-Ting Yuan,
  • Luis C. Ho,
  • Junxian Wang,
  • Linhua Jiang,
  • James E. Rhoads,
  • Sangeeta Malhotra,
  • L. Felipe Barrientos,
  • Isak Wold,
  • Leopoldo Infante,
  • Shuairu Zhu,
  • Xiang Ji,
  • Xiaodan Fu

DOI
https://doi.org/10.3847/2041-8213/adaaf1
Journal volume & issue
Vol. 980, no. 2
p. L34

Abstract

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Recently, the James Webb Space Telescope has revealed a new class of high-redshift (high- z , z > 4) compact galaxies that are red in the rest-frame optical and blue in the rest-frame UV with V-shaped spectral energy distributions (SEDs), referred to as “little red dots” (LRDs). It is very likely that LRDs host obscured broad-line active galactic nuclei (AGNs). In the meanwhile, Green Pea galaxies (GPs), which are compact dwarf galaxies at low redshift, share various similar properties with high-redshift star-forming galaxies. Here, we aim to find the connection between the LRDs and GPs hosting broad-line AGNs (BLGPs). With a sample of 19 BLGPs obtained from our previous work, we further identify seven GPs with V-shaped rest-frame UV-to-optical SEDs that are likely local analogs to LRDs. These V-shaped BLGPs exhibit faint UV absolute magnitudes and sub-Eddington rates similar to those of LRDs. Three of them occupy a similar region to LRDs in the Baldwin–Philips–Terlevich diagram, suggesting they have similar ionization conditions and gas-phase metallicities to LRDs. These similarities suggest that V-shaped BLGPs can be taken as local analogs of high-redshift LRDs. In addition, most (16/19) BLGPs, including six V-shaped BLGPs, host overmassive black holes (BHs) above the local M _BH – M _* relation, making it the first sample of galaxies hosting overmassive BHs at z < 0.4. These findings will help us learn more about the formation and coevolution of early galaxies and BHs.

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