Solar abundance of iridium
By a method of spectrum synthesis, which yields log gfA, where g is the statistical weight of the lower level, f is the oscillator strength, and A is the abundance, an attempt is made to deduce the solar iridium abundance from one relatively unblended, but fairly weak IrI line, λ 3220.78 Å. If the C...
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
1976
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| Sujets: | |
| Accès en ligne: | https://ncbi.nlm.nih.govhttps://pmc.ncbi.nlm.nih.gov/articles/PMC335885/ https://ncbi.nlm.nih.govhttps://pubmed.ncbi.nlm.nih.gov/16578735/ https://ncbi.nlm.nih.govhttps://doi.org/10.1073/pnas.73.2.269 |
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