Nebular and auroral emission lines of [Cl iii] in the optical spectra of planetary nebulae

Electron impact excitation rates in Cl III, recently determined with the R-matrix code, are used to calculate electron temperature (T(e)) and density (N(e)) emission line ratios involving both the nebular (5517.7, 5537.9 Å) and auroral (8433.9, 8480.9, 8500.0 Å) transitions. A comparison of these re...

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Détails bibliographiques
Auteurs principaux: Keenan, Francis P., Aller, Lawrence H., Ramsbottom, Catherine A., Bell, Kenneth L., Crawford, Fergal L., Hyung, Siek
Format: Artigo
Langue:Inglês
Publié: The National Academy of Sciences 2000
Sujets:
Physical Sciences
Accès en ligne:https://ncbi.nlm.nih.gov/pmc/articles/PMC18270/
https://ncbi.nlm.nih.gov/pubmed/10759562
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