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G. Favole, Violeta González-Pérez, Y. Ascasíbar, Pablo Corcho-Caballero, Antonio D. Montero-Dorta, Andrew Benson, Johan Comparat, S. A. Cora, Darren Croton, H. Guo · 2023 · arXiv (Cornell University) · DOI 10.48550/arxiv.2303.11031 · arXiv 2303.11031

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Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model

astro-ph.GA · 2026-05-07 · conditional · novelty 7.0

Extreme z>3 emission-line ratios are reproduced only by combining harder ionizing spectra, ionization parameters from massive star clusters, and enhanced nitrogen abundances.

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Origins of Extreme Emission-Line Ratios in z > 3 Galaxies: Insights from the Lumen Model astro-ph.GA · 2026-05-07 · conditional · none · ref 97
Extreme z>3 emission-line ratios are reproduced only by combining harder ionizing spectra, ionization parameters from massive star clusters, and enhanced nitrogen abundances.

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