Sulphur abundance determinations in star-forming regions : I. Ionization correction factor
In this work, we used a grid of photoionization models combined with stellar population synthesis models to derive reliable ionization correction factors (ICFs) for the sulphur in star-forming regions. These models cover a large range of nebular parameters and yielding ionic abundances in consonance...
Guardado en:
| Autores principales: | Dors, Oli L., Pérez Montero, E., Hägele, Guillermo Federico, Cardaci, Mónica Viviana, Krabbe, A. C. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2016
|
| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93863 https://academic.oup.com/mnras/article-abstract/456/4/4407/1036277?redirectedFrom=fulltext https://ri.conicet.gov.ar/handle/11336/35921 |
| Aporte de: |
Ejemplares similares
-
Optical and mid-infrared neon abundance determinations in star-forming regions
por: Dors Junior, Oli L., et al.
Publicado: (2013) -
Effective temperature of ionizing stars of extragalactic HII regions
por: Dors, Oli LUiz, et al.
Publicado: (2017) -
Analysing derived metallicities and ionization parameters from model-based determinations in ionized gaseous nebulae
por: Dors Junior, O. L., et al.
Publicado: (2011) -
Chemical abundances in Seyfert galaxies – VII. Direct abundance determination of neon based on optical and infrared emission lines
por: Armah, Mark, et al.
Publicado: (2021) -
Chemical abundances of Seyfert 2 AGNs – III. Reducing the oxygen abundance discrepancy
por: Dors, Oli L., et al.
Publicado: (2020)