Resumen
We carefully consider numerous explanations for the sulfur abundance anomaly in planetary nebulae. No one rationale appears to be satisfactory, and we suggest that the ultimate explanation is likely to be a heretofore unidentified feature of the nebular gas which significantly impacts the sulfur ionization correction factor.
| Idioma original | English |
|---|---|
| Título de la publicación alojada | Planetary Nebulae |
| Subtítulo de la publicación alojada | An Eye to the Future |
| Páginas | 384-385 |
| Número de páginas | 2 |
| Edición | S283 |
| DOI | |
| Estado | Published - jul 2011 |
Serie de la publicación
| Nombre | Proceedings of the International Astronomical Union |
|---|---|
| Número | S283 |
| Volumen | 7 |
| ISSN (versión impresa) | 1743-9213 |
| ISSN (versión digital) | 1743-9221 |
Nota bibliográfica
Funding Information:We gratefully acknowledge support from the US-NSF (RBCH, GJF) and the NCI National Facility at the Australian National University (AIK). We also thank Matthew Hosak for computing the photoionization models and Karen Kwitter for the use of her PN database.
Financiación
We gratefully acknowledge support from the US-NSF (RBCH, GJF) and the NCI National Facility at the Australian National University (AIK). We also thank Matthew Hosak for computing the photoionization models and Karen Kwitter for the use of her PN database.
| Financiadores |
|---|
| US NSF |
| National Computational Infrastructure |
ODS de las Naciones Unidas
Este resultado contribuye a los siguientes Objetivos de Desarrollo Sostenible
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Good health and well being
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science
Huella
Profundice en los temas de investigación de 'The curious conundrum regarding sulfur and oxygen abundances in planetary nebulae'. En conjunto forman una huella única.Citar esto
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