On the production of He, C, and N by low- and intermediate-mass stars: a comparison of observed and model-predicted planetary nebula abundances
The primary goal of this paper is to make a direct comparison between the measured and model-predicted abundances of He, C, and N in a sample of 35 well-observed Galactic planetary nebulae (PNe). All observations, data reductions, and abundance determinations were performed in house to ensure maximu...
Guardado en:
| Autores principales: | Henry, R. B. C., Stephenson, B. G., Miller Bertolami, Marcelo Miguel, Kwitter, K. B., Balick, B. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2018
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/93706 https://academic.oup.com/mnras/article-abstract/473/1/241/4107117 https://ri.conicet.gov.ar/handle/11336/82516 |
| Aporte de: |
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