[Fe IV] Emission in Ionized Nebulae
I present the results of an analysis of [Fe IV] emission in several ionized nebulae, which is based on new identifications and previous measurements of [Fe IV] lines. The Fe abundances obtained by adding the abundances of the relevant Fe ions (mainly Fe++ and Fe3+) are found to be lower, by factors...
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| Udgivet i: | Revista Mexicana de Astronomía y Astrofísica |
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| Hovedforfatter: | |
| Format: | Artigo |
| Sprog: | Inglês |
| Udgivet: |
Universidad Nacional Autónoma de México
2003
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| Fag: | |
| Online adgang: | https://www.redalyc.org/articulo.oa?id=57101826 |
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