Nature and chemical abundances of a sample of Lyman-α emitter objects at high redshift
We built a grid of photoionization models and compiled already available observational emission line intensities (1000 < λ(Å) < 2000) of confirmed star formation regions and Active Galactic Nucleus (AGNs) in order to classify five Lyα emitter (LAE) objects at high redshift (5.7 < z < 7.2...
Guardado en:
| Autores principales: | Dors, Oli L., Agarwal, B., Hägele, Guillermo Federico, Cardaci, Monica Viviana, Rydberg, Claes Erik, Riffel, R. A., Oliveira, A. S., Krabbe, A. C. |
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| Formato: | Articulo Preprint |
| Lenguaje: | Inglés |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93617 https://academic.oup.com/mnras/article/479/2/2294/5045259 |
| Aporte de: |
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