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The curious conundrum regarding sulfur and oxygen abundances in planetary nebulae

Producción científica: Conference contributionrevisión exhaustiva

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 originalEnglish
Título de la publicación alojadaPlanetary Nebulae
Subtítulo de la publicación alojadaAn Eye to the Future
Páginas384-385
Número de páginas2
EdiciónS283
DOI
EstadoPublished - jul 2011

Serie de la publicación

NombreProceedings of the International Astronomical Union
NúmeroS283
Volumen7
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

    1. Good health and well being
      Good health and well being

    ASJC Scopus subject areas

    • Astronomy and Astrophysics
    • Space and Planetary Science

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