Chemical Composition of Nebulosities in the Magellanic Clouds

From photoelectric spectrophotometric data secured at Cerro Tololo Interamerican Observatory we have attempted to derive electron densities and temperatures, ionic concentrations, and chemical abundances of He, C, N, O, Ne, S, and Ar in nebulosities in the Magellanic Clouds. Although 10 distinct neb...

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Dades bibliogràfiques

Publicat a:	Proc Natl Acad Sci U S A
Autors principals:	Aller, L. H., Czyzak, S. J., Keyes, C. D., Boeshaar, G.
Format:	Artigo
Idioma:	Inglês
Publicat:	National Academy of Sciences 1974
Matèries:	Physical Sciences: Astronomy
Accés en línia:	https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC433913/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/16592199/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.71.11.4496
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