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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...
Tallennettuna:
| Julkaisussa: | Proc Natl Acad Sci U S A |
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| Päätekijät: | , , , |
| Aineistotyyppi: | Artigo |
| Kieli: | Inglês |
| Julkaistu: |
National Academy of Sciences
1974
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| Aiheet: | |
| Linkit: | 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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