No top-heavy stellar initial mass function needed: the ionizing radiation of GS9422 can be powered by a mixture of AGN and stars

Ähnliche Einträge

• Resolving the nature and putative nebular emission of GS9422: an obscured AGN without exotic stars
  von: Tacchella, Sandro, et al.
  Veröffentlicht: (2024)
• Sub-millimeter galaxies in hierarchical models: revisiting the need for a top-heavy stellar initial mass function with Bayesian optimisation
  von: Elliott, Edward, et al.
  Veröffentlicht: (2025)
• Cue: A Fast and Flexible Photoionization Emulator for Modeling Nebular Emission Powered By Almost Any Ionizing Source
  von: Li, Yijia, et al.
  Veröffentlicht: (2024)
• Mirror images of lensed star clusters with mismatched spectral energy distributions: A possible signature of top-heavy stellar initial mass functions and extreme stars in high-redshift star clusters
  von: Zackrisson, Erik, et al.
  Veröffentlicht: (2026)
• JWST Reveals Widespread AGN-Driven Neutral Gas Outflows in Massive z ~ 2 Galaxies
  von: Davies, Rebecca L., et al.
  Veröffentlicht: (2023)