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Chemical composition of high-excitation planetaries
Nebular spectral line intensities measured mostly in the optical region, but also in the IR and satellite UV (where possible), are used to derive plasma diagnostics and ionic concentrations n (X(i))/n(H(+)). Then, we use theoretical nebular models to represent as closely as possible certain excitati...
Enregistré dans:
| Publié dans: | Proc Natl Acad Sci U S A |
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| Auteurs principaux: | , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
National Academy of Sciences
1981
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| Sujets: | |
| Accès en ligne: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC348722/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/16593076/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.78.9.5266 |
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