Strong rest-UV emission lines in a "little red dot" AGN at $z=7$: Early SMBH growth alongside compact massive star formation?

Documenti analoghi

• Tentative detection of neutral gas in a Little Red Dot at $z=4.46$
  di: Akins, Hollis B., et al.
  Pubblicazione: (2025)
• COSMOS-Web: The over-abundance and physical nature of "little red dots"--Implications for early galaxy and SMBH assembly
  di: Akins, Hollis B., et al.
  Pubblicazione: (2024)
• Silencing the Giant: Evidence of AGN Feedback and Quenching in a Little Red Dot at z = 4.13
  di: Kokorev, Vasily, et al.
  Pubblicazione: (2024)
• Modeling Galaxies in the Early Universe with Supernova Dust Attenuation
  di: McKinney, Jed, et al.
  Pubblicazione: (2025)
• Dust in Little Red Dots
  di: Casey, Caitlin M., et al.
  Pubblicazione: (2024)