Investigating the ionization mechanisms powering the extreme emission lines in metal-poor galaxies

arXiv:2609.28329 · astro-ph.GA · Submitted 2026-09-23 · Read on arXiv

astro-ph.GA

Submitted: 2026-09-23

Updated: 2026-09-23

Terminology

AGN — 42× in this paper · explained in 1 episode
Metallicity — 19× in this paper · explained in 3 episodes
Calibration — 12× in this paper · explained in 7 episodes
Aperture — 8× in this paper · explained in 1 episode
Abundance — 6× in this paper · explained in 1 episode
Trace — 3× in this paper · explained in 2 episodes
Core — 2× in this paper · explained in 2 episodes
Diagnostic Tools — 2× in this paper · explained in 2 episodes
Star Formation Rate (SFR) — 2× in this paper · explained in 5 episodes
Alignment — 1× in this paper · explained in 1 episode
Aperture Correction — 1× in this paper · explained in 1 episode
Consistency — 1× in this paper · explained in 3 episodes
Degeneracy — 1× in this paper · explained in 3 episodes
Fine-Tuning — 1× in this paper · explained in 5 episodes
Ionization Parameter (U) — 1× in this paper · explained in 2 episodes
Medium-Resolution Spectrometer — 1× in this paper
Population Synthesis — 1× in this paper · explained in 2 episodes
Self-consistency — 1× in this paper · explained in 2 episodes
Stellar Feedback — 1× in this paper · explained in 2 episodes
Verification — 1× in this paper · explained in 2 episodes

Sources

JWST/NIRSpec Reveals Diverse Nuclear Environments in Dwarf Galaxies Hosting AGN

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