Delayed Feedback in High- z Starbursts Revealed by Lyman- alpha Profiles and Metal Line Diagnostics

arXiv:2506.20422 · astro-ph.GA · Submitted 2025-06-25 · Read on arXiv

astro-ph.GA

Submitted: 2025-06-25

Updated: 2026-09-01

Terminology

alpha — 10× in this paper · explained in 1 episode
Aperture — 9× in this paper · explained in 1 episode
Core — 8× in this paper · explained in 2 episodes
AGN — 6× in this paper · explained in 1 episode
Gravitational Lensing — 5× in this paper · explained in 2 episodes
Metallicity — 5× in this paper · explained in 3 episodes
Stellar Feedback — 5× in this paper · explained in 2 episodes
Abundance — 4× in this paper · explained in 1 episode
Dust Attenuation — 4× in this paper · explained in 2 episodes
Trace — 4× in this paper · explained in 2 episodes
Multi-Unit Spectroscopic Explorer — 2× in this paper
Spectral Signature — 2× in this paper · explained in 2 episodes
Accuracy — 1× in this paper · explained in 1 episode
Active Galactic Nuclei (AGN) — 1× in this paper · explained in 1 episode
Calibration — 1× in this paper · explained in 7 episodes
Degeneracy — 1× in this paper · explained in 3 episodes
Homogeneity — 1× in this paper · explained in 2 episodes
Robustness — 1× in this paper · explained in 5 episodes
Signal-to-noise ratio (SNR) — 1× in this paper · explained in 2 episodes

Sources

Anatomy of a z=6 Lyman-{\alpha} emitter down to parsec scales: extreme UV slopes, metal-poor regions and possibly leaking star clusters

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